This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Vend14,2461124.9555,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Vend14 20260325.4555 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:29.24 +44:32:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 10.51 21:00:49.41 +47:42:57.7
88.28710 0.97245 galactic Cyg Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2108+47.7210 | 21:00:49.35 +47:42:58.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2108+47.7210,2461124.9555,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2108+47.7210 20260325.4555 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:49.41 +47:42:57.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163897127531223552,2461124.9555,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163897127531223552 20260325.4555 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:34.83 +47:23:01.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 10.52 21:01:04.14 +47:53:15.6
88.44334 1.05464 galactic Cyg Second-epoch detections are separated by 0.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2482+47.8853 | 21:01:04.10 +47:53:16.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.030 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2482+47.8853,2461124.9555,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2482+47.8853 20260325.4555 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:04.14 +47:53:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 10.46 21:00:36.46 +47:54:44.4
88.41091 1.12905 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163973577951574784 | 21:00:36.30 +47:54:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.261+/-0.031 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163973577951574784,2461124.9555,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163973577951574784 20260325.4555 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:36.46 +47:54:44.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
PMAK V30,2461124.9555,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PMAK V30 20260325.4555 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:56.50 +43:29:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0573 Cyg,2461124.9555,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0573 Cyg 20260325.4555 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:45.05 +47:24:08.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 10.47 21:00:33.37 +47:29:25.6
88.08769 0.85772 galactic Cyg Second-epoch detections are separated by 0.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1536+47.4852 | 21:00:33.28 +47:29:26.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1536+47.4852,2461124.9555,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1536+47.4852 20260325.4555 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:33.37 +47:29:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211127.99+450614.4,2461124.9555,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211127.99+450614.4 20260325.4555 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:11:30.25 +45:06:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.37 21:10:53.92 +47:22:42.5
89.17810 -0.51426 galactic Cyg Second-epoch detections are separated by 6.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.6989+47.3761 | 21:10:51.68 +47:22:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.879+/-0.073 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J317.6989+47.3761,2461124.9555,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.6989+47.3761 20260325.4555 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:53.92 +47:22:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.14 21:00:44.45 +46:06:59.7
87.07495 -0.07122 galactic Cyg Second-epoch detections are separated by 1.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1594+46.1060 | 21:00:42.60 +46:06:19.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1594+46.1060,2461124.9555,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1594+46.1060 20260325.4555 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:44.45 +46:06:59.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210119.27+464104.1,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210119.27+464104.1 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:18.55 +46:41:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.05 21:01:54.64 +42:42:36.2
84.65349 -2.47712 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:54.64 +42:42:36.2 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:54.64 +42:42:36.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.87 21:01:46.19 +46:09:51.8
87.22855 -0.17351 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4321+46.1731 | 21:01:43.72 +46:10:23.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.112+/-0.034 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4321+46.1731,2461124.9555,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4321+46.1731 20260325.4555 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:46.19 +46:09:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.53 21:01:50.41 +47:55:02.9
88.55112 0.97731 galactic Cyg Second-epoch detections are separated by 0.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2165460701777922176 | 21:01:50.38 +47:55:04.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.398+/-0.026 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2165460701777922176,2461124.9555,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2165460701777922176 20260325.4555 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:50.41 +47:55:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0578 Cyg,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0578 Cyg 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:08.42 +48:51:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163628709266423296,2461124.9555,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163628709266423296 20260325.4555 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:38.41 +46:18:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213928.71+420437.4,2461124.9555,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213928.71+420437.4 20260325.4555 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:28.77 +42:04:37.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.62 21:02:04.36 +43:52:52.1
85.55187 -1.72457 galactic Cyg Second-epoch detections are separated by 2.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5300+43.8805 | 21:02:04.36 +43:52:52.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.545+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5300+43.8805,2461124.9555,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5300+43.8805 20260325.4555 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:04.36 +43:52:52.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.04 21:00:24.54 +47:27:40.6
88.04936 0.85723 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1034+47.4651 | 21:00:24.54 +47:27:40.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.328+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1034+47.4651,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1034+47.4651 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:24.54 +47:27:40.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.19 21:02:33.31 +46:38:50.7
87.68006 0.04506 galactic Cyg Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6376+46.6503 | 21:02:33.31 +46:38:50.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.147+/-0.032 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6376+46.6503,2461124.9555,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6376+46.6503 20260325.4555 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:33.31 +46:38:50.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J215856.74+432257.1,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215856.74+432257.1 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:56.55 +43:22:56.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.30 21:41:38.76 +42:32:27.2
89.71597 -7.76738 galactic Cyg Second-epoch detections are separated by 1.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:38.76 +42:32:27.2 (user input) | T | P | (position from user input) J-Ks=1.152+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:38.76 +42:32:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.30 21:00:44.11 +46:15:56.8
87.18650 0.02785 galactic Cyg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1829+46.2821 | 21:00:44.73 +46:16:41.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1829+46.2821,2461124.9555,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1829+46.2821 20260325.4555 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:44.11 +46:15:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972885260262133632,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972885260262133632 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:31.19 +43:06:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214445.79+432820.8,2461124.9555,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214445.79+432820.8 20260325.4555 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:45.84 +43:28:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:01:11.17 +46:11:52.3
87.18690 -0.07557 galactic Cyg Second-epoch detections are separated by 0.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2970+46.2048 | 21:01:11.17 +46:11:52.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.082+/-0.037 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2970+46.2048,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2970+46.2048 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:11.17 +46:11:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.52 21:00:16.89 +47:16:05.1
87.88967 0.74635 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0638+47.2697 | 21:00:16.89 +47:16:05.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.341+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0638+47.2697,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0638+47.2697 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:16.89 +47:16:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.93 22:07:50.22 +48:57:43.0
97.34077 -5.60849 galactic Lac Second-epoch detections are separated by 1.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976568143184204032 | 22:07:50.43 +48:57:45.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976568143184204032,2461124.9555,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976568143184204032 20260325.4555 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:50.22 +48:57:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.73 21:04:49.68 +44:12:50.6
86.13005 -1.87287 galactic Cyg Second-epoch detections are separated by 2.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.2066+44.2146 | 21:04:49.68 +44:12:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.295+/-0.030 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.2066+44.2146,2461124.9555,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.2066+44.2146 20260325.4555 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:49.68 +44:12:50.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.60 21:02:18.90 +47:12:14.3
88.06948 0.44481 galactic Cyg Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5925+47.2022 | 21:02:18.90 +47:12:14.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.334+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5925+47.2022,2461124.9555,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5925+47.2022 20260325.4555 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:18.90 +47:12:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.77 21:00:42.01 +46:29:12.5
87.34876 0.17806 galactic Cyg Second-epoch detections are separated by 0.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1750+46.4871 | 21:00:42.01 +46:29:12.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.205+/-0.032 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1750+46.4871,2461124.9555,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1750+46.4871 20260325.4555 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:42.01 +46:29:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.72 21:01:26.19 +46:58:32.2
87.79931 0.40580 galactic Cyg Second-epoch detections are separated by 0.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:26.19 +46:58:32.2 (user input) | T | P | (position from user input) J-Ks=0.208+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:26.19 +46:58:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.69 22:12:21.99 +49:22:24.0
98.18675 -5.70161 galactic Lac Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1975941009240008448 | 22:12:22.01 +49:22:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.141+/-0.035 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975941009240008448,2461124.9555,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1975941009240008448 20260325.4555 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:21.99 +49:22:24.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.60 21:01:27.70 +47:17:20.1
88.03732 0.60960 galactic Cyg Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:27.70 +47:17:20.1 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:27.70 +47:17:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.64 21:01:27.53 +47:21:36.3
88.09042 0.65698 galactic Cyg Second-epoch detections are separated by 1.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3732+47.3685 | 21:01:27.53 +47:21:36.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.376+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3732+47.3685,2461124.9555,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3732+47.3685 20260325.4555 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:27.53 +47:21:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.41 21:00:31.68 +47:20:36.3
87.97389 0.76448 galactic Cyg Second-epoch detections are separated by 1.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1313+47.3438 | 21:00:31.68 +47:20:36.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.426+/-0.033 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1313+47.3438,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1313+47.3438 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:31.68 +47:20:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.48 21:01:21.65 +47:02:22.6
87.83883 0.45776 galactic Cyg Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:21.65 +47:02:22.6 (user input) | T | P | (position from user input) J-Ks=1.318+/-0.033 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:21.65 +47:02:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.58 21:03:12.16 +43:19:50.4
85.27529 -2.24270 galactic Cyg Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:12.16 +43:19:50.4 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.029 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:12.16 +43:19:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.62 21:00:35.25 +47:07:08.6
87.81170 0.60912 galactic Cyg Second-epoch detections are separated by 0.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163868020526987136 | 21:00:35.21 +47:07:09.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.439+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163868020526987136,2461124.9555,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163868020526987136 20260325.4555 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:35.25 +47:07:08.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.54 21:03:50.43 +47:55:38.6
88.78107 0.73331 galactic Cyg Second-epoch detections are separated by 0.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:50.43 +47:55:38.6 (user input) | T | P | (position from user input) J-Ks=0.234+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:50.43 +47:55:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:45.23 +46:59:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214318.97+435757.5,2461124.9555,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214318.97+435757.5 20260325.4555 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:18.98 +43:57:57.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.47 21:01:10.16 +46:21:53.8
87.31049 0.03691 galactic Cyg Second-epoch detections are separated by 3.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:10.16 +46:21:53.8 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:10.16 +46:21:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.55 21:04:25.79 +44:12:40.7
86.08033 -1.82160 galactic Cyg Second-epoch detections are separated by 0.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.1066+44.2146 | 21:04:25.79 +44:12:40.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.579+/-0.029 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.1066+44.2146,2461124.9555,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.1066+44.2146 20260325.4555 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:25.79 +44:12:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.62 21:00:39.72 +47:21:26.7
87.99938 0.75663 galactic Cyg Second-epoch detections are separated by 0.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1646+47.3534 | 21:00:39.72 +47:21:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.336+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1646+47.3534,2461124.9555,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1646+47.3534 20260325.4555 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:39.72 +47:21:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.66 21:02:48.65 +47:30:14.0
88.34962 0.58093 galactic Cyg Second-epoch detections are separated by 0.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7006+47.5069 | 21:02:48.65 +47:30:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.367+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7006+47.5069,2461124.9555,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7006+47.5069 20260325.4555 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:48.65 +47:30:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.29 21:41:17.27 +43:12:56.5
90.11674 -7.21803 galactic Cyg Second-epoch detections are separated by 0.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972934356027689984 | 21:41:17.27 +43:12:58.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.229+/-0.029 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972934356027689984,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972934356027689984 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:17.27 +43:12:56.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.32 21:01:45.98 +44:02:42.1
85.63834 -1.57482 galactic Cyg Second-epoch detections are separated by 3.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4376+44.0475 | 21:01:45.98 +44:02:42.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.435+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4376+44.0475,2461124.9555,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4376+44.0475 20260325.4555 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:45.98 +44:02:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.30 21:40:51.65 +43:04:31.4
89.96424 -7.27155 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2308+43.0799 | 21:40:51.65 +43:04:31.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.830+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2308+43.0799,2461124.9555,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2308+43.0799 20260325.4555 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:51.65 +43:04:31.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.41 21:01:38.07 +43:06:18.6
84.91684 -2.17806 galactic Cyg Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:38.07 +43:06:18.6 (user input) | T | P | (position from user input) J-Ks=0.471+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:38.07 +43:06:18.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163538377513935360,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163538377513935360 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:04.56 +46:16:22.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J220655.41+484619.1,2461124.9555,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J220655.41+484619.1 20260325.4555 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:55.12 +48:46:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.18 21:46:46.23 +44:12:42.3
91.52869 -7.11328 galactic Cyg Second-epoch detections are separated by 1.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.6925+44.2120 | 21:46:46.21 +44:12:43.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.285+/-0.035 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.6925+44.2120,2461124.9555,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.6925+44.2120 20260325.4555 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:46.23 +44:12:42.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.64 21:06:52.19 +43:27:55.1
85.82125 -2.64809 galactic Cyg Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:06:52.19 +43:27:55.1 (user input) | T | P | (position from user input) J-Ks=1.393+/-0.036 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:06:52.19 +43:27:55.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UCAC4 673-106048,2461124.9555,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UCAC4 673-106048 20260325.4555 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:37.38 +44:29:47.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 10.96 21:00:20.58 +47:45:34.2
88.26660 1.06187 galactic Cyg Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0850+47.7652 | 21:00:20.50 +47:45:35.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.849+/-0.025 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0850+47.7652,2461124.9555,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0850+47.7652 20260325.4555 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:20.58 +47:45:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.60 21:01:56.64 +46:52:04.3
87.77579 0.26954 galactic Cyg Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:56.64 +46:52:04.3 (user input) | T | P | (position from user input) J-Ks=0.255+/-0.039 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:56.64 +46:52:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.48 21:46:01.76 +43:46:35.9
91.14208 -7.35822 galactic Cyg Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:01.76 +43:46:35.9 (user input) | T | P | (position from user input) J-Ks=0.665+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:01.76 +43:46:35.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.69 21:02:23.13 +47:46:41.1
88.50726 0.81645 galactic Cyg Second-epoch detections are separated by 2.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5965+47.7786 | 21:02:23.13 +47:46:41.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.552+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5965+47.7786,2461124.9555,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5965+47.7786 20260325.4555 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:23.13 +47:46:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.12 21:00:37.18 +47:50:17.6
88.35646 1.07872 galactic Cyg Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1627+47.8346 | 21:00:39.54 +47:49:42.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1627+47.8346,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1627+47.8346 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:37.18 +47:50:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:01:22.53 +46:40:19.8
87.56462 0.21316 galactic Cyg Second-epoch detections are separated by 0.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3529+46.6702 | 21:01:26.32 +46:40:21.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.785+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3529+46.6702,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3529+46.6702 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:22.53 +46:40:19.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.53 21:44:15.59 +43:58:12.3
91.02525 -7.00371 galactic Cyg Second-epoch detections are separated by 2.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:15.59 +43:58:12.3 (user input) | T | P | (position from user input) J-Ks=1.122+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:15.59 +43:58:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.38 21:01:39.93 +43:55:06.2
85.53129 -1.64492 galactic Cyg Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4161+43.9187 | 21:01:39.93 +43:55:06.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.435+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4161+43.9187,2461124.9555,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4161+43.9187 20260325.4555 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:39.93 +43:55:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.34 21:02:03.65 +47:07:10.0
87.97753 0.42117 galactic Cyg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:03.65 +47:07:10.0 (user input) | T | P | (position from user input) J-Ks=0.246+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:03.65 +47:07:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.62 21:00:55.95 +47:31:10.3
88.15145 0.82908 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163906026703864448 | 21:00:55.95 +47:31:11.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163906026703864448,2461124.9555,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163906026703864448 20260325.4555 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:55.95 +47:31:10.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 10.99 21:01:05.78 +47:40:22.0
88.28486 0.90941 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163954027260435328 | 21:01:05.68 +47:40:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.255+/-0.039 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163954027260435328,2461124.9555,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163954027260435328 20260325.4555 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:05.78 +47:40:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:08.77 +47:34:15.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.81 21:01:24.29 +47:48:25.7
88.42004 0.95916 galactic Cyg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3580+47.8106 | 21:01:24.17 +47:48:27.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.066+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3580+47.8106,2461124.9555,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3580+47.8106 20260325.4555 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:24.29 +47:48:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.59 21:00:46.59 +47:34:58.1
88.18168 0.89059 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1938+47.5834 | 21:00:46.59 +47:34:58.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1938+47.5834,2461124.9555,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1938+47.5834 20260325.4555 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:46.59 +47:34:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:00:41.62 +47:23:33.7
88.02945 0.77584 galactic Cyg Second-epoch detections are separated by 1.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:41.62 +47:23:33.7 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.029 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:41.62 +47:23:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.64 21:01:36.59 +47:34:59.8
88.27480 0.78534 galactic Cyg Second-epoch detections are separated by 0.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:36.59 +47:34:59.8 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:36.59 +47:34:59.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163906404660991232,2461124.9555,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163906404660991232 20260325.4555 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:01.14 +47:34:18.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.56 21:00:24.57 +47:20:44.2
87.96233 0.78104 galactic Cyg Second-epoch detections are separated by 1.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1055+47.3465 | 21:00:24.57 +47:20:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.359+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1055+47.3465,2461124.9555,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1055+47.3465 20260325.4555 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:24.57 +47:20:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163473059648499968,2461124.9555,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163473059648499968 20260325.4555 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:56.58 +45:47:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.22 21:01:45.91 +43:27:30.6
85.19793 -1.96242 galactic Cyg Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4407+43.4587 | 21:01:45.77 +43:27:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.243+/-0.027 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4407+43.4587,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4407+43.4587 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:45.91 +43:27:30.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.01 21:01:32.15 +46:02:08.2
87.10512 -0.22824 galactic Cyg Second-epoch detections are separated by 0.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3811+46.0321 | 21:01:32.15 +46:02:08.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.426+/-0.045 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3811+46.0321,2461124.9555,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3811+46.0321 20260325.4555 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:32.15 +46:02:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.23 21:01:01.95 +47:48:45.1
88.38282 1.00968 galactic Cyg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2504+47.8067 | 21:01:01.95 +47:48:45.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.349+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2504+47.8067,2461124.9555,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2504+47.8067 20260325.4555 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:01.95 +47:48:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.22 21:01:51.97 +46:37:43.6
87.58774 0.12130 galactic Cyg Second-epoch detections are separated by 0.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4620+46.6313 | 21:01:51.97 +46:37:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.303+/-0.049 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4620+46.6313,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4620+46.6313 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:51.97 +46:37:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.42 21:00:43.92 +47:19:26.9
87.98216 0.72578 galactic Cyg Second-epoch detections are separated by 0.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:43.92 +47:19:26.9 (user input) | T | P | (position from user input) J-Ks=0.991+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:43.92 +47:19:26.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:02:22.54 +47:12:04.9
88.07435 0.43536 galactic Cyg Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5925+47.2022 | 21:02:22.54 +47:12:04.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5925+47.2022,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5925+47.2022 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:22.54 +47:12:04.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.38 21:03:21.25 +46:58:15.0
88.01262 0.15774 galactic Cyg Second-epoch detections are separated by 1.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163677671895348480 | 21:03:18.14 +46:58:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163677671895348480,2461124.9555,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163677671895348480 20260325.4555 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:21.25 +46:58:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.26 21:01:25.22 +46:51:10.3
87.70534 0.32677 galactic Cyg Second-epoch detections are separated by 3.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3551+46.8529 | 21:01:25.22 +46:51:10.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.791+/-0.054 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3551+46.8529,2461124.9555,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3551+46.8529 20260325.4555 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:25.22 +46:51:10.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.70 21:45:20.75 +44:00:03.1
91.19469 -7.10779 galactic Cyg Second-epoch detections are separated by 3.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.3265+43.9966 | 21:45:20.75 +44:00:03.1 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.792+/-0.025 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.3265+43.9966,2461124.9555,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.3265+43.9966 20260325.4555 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:20.75 +44:00:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.91 21:01:12.60 +46:58:06.7
87.76847 0.43013 galactic Cyg Second-epoch detections are separated by 1.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2832+46.9721 | 21:01:12.41 +46:58:08.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2832+46.9721,2461124.9555,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2832+46.9721 20260325.4555 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:12.60 +46:58:06.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:00:46.75 +45:41:15.1
86.75668 -0.35904 galactic Cyg Second-epoch detections are separated by 1.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1878+45.6979 | 21:00:46.75 +45:41:15.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.381+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1878+45.6979,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1878+45.6979 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:46.75 +45:41:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:02:09.50 +47:08:39.4
88.00712 0.42520 galactic Cyg Second-epoch detections are separated by 0.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:09.50 +47:08:39.4 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:09.50 +47:08:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J210132.28+471319.4,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J210132.28+471319.4 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:32.39 +47:13:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.90 21:00:32.39 +47:01:19.4
87.73336 0.55134 galactic Cyg Second-epoch detections are separated by 0.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1270+47.0122 | 21:00:32.24 +47:01:20.8 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.320+/-0.042 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1270+47.0122,2461124.9555,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1270+47.0122 20260325.4555 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:32.39 +47:01:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.36 21:01:27.88 +46:42:29.0
87.60166 0.22539 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3659+46.7081 | 21:01:27.88 +46:42:29.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.208+/-0.038 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3659+46.7081,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3659+46.7081 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:27.88 +46:42:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.96 21:01:02.48 +45:57:30.3
86.99044 -0.21472 galactic Cyg Second-epoch detections are separated by 0.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2600+45.9587 | 21:01:02.41 +45:57:31.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.239+/-0.036 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2600+45.9587,2461124.9555,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2600+45.9587 20260325.4555 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:02.48 +45:57:30.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163889838957918208,2461124.9555,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163889838957918208 20260325.4555 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:15.01 +47:25:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163668394765720576,2461124.9555,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163668394765720576 20260325.4555 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:52.24 +46:46:50.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.33 21:03:13.44 +47:09:13.3
88.13443 0.29592 galactic Cyg Second-epoch detections are separated by 1.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.8058+47.1452 | 21:03:13.44 +47:09:13.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.072+/-0.036 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.8058+47.1452,2461124.9555,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.8058+47.1452 20260325.4555 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:13.44 +47:09:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:01:11.17 +47:15:47.2
87.98708 0.62764 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:11.17 +47:15:47.2 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:11.17 +47:15:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:43:13.11 +42:38:46.9
90.00574 -7.87903 galactic Cyg Second-epoch detections are separated by 3.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.7948+42.6364 | 21:43:13.11 +42:38:46.9 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.898+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.7948+42.6364,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7948+42.6364 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:13.11 +42:38:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163477045377584256,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163477045377584256 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:01.71 +45:55:07.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.06 21:01:51.20 +47:22:01.5
88.13985 0.61149 galactic Cyg Second-epoch detections are separated by 1.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163888602006681088 | 21:01:51.15 +47:22:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.230+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163888602006681088,2461124.9555,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163888602006681088 20260325.4555 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:51.20 +47:22:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:43:18.09 +42:50:50.1
90.15064 -7.73768 galactic Cyg Second-epoch detections are separated by 2.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8181+42.8368 | 21:43:18.09 +42:50:50.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.342+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8181+42.8368,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8181+42.8368 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:18.09 +42:50:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.50 21:03:11.28 +44:29:58.6
86.14757 -1.46400 galactic Cyg Second-epoch detections are separated by 0.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:11.28 +44:29:58.6 (user input) | T | P | (position from user input) J-Ks=0.619+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:11.28 +44:29:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:27.86 +47:11:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163630495972973312,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163630495972973312 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:56.03 +46:21:42.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.14 21:03:30.15 +46:45:00.1
87.86468 -0.00813 galactic Cyg Second-epoch detections are separated by 0.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.8718+46.7505 | 21:03:30.15 +46:45:00.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.099+/-0.025 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.8718+46.7505,2461124.9555,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.8718+46.7505 20260325.4555 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:30.15 +46:45:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.11 21:45:07.04 +43:56:01.9
91.11927 -7.13186 galactic Cyg Second-epoch detections are separated by 0.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.2894+43.9366 | 21:45:07.04 +43:56:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.707+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.2894+43.9366,2461124.9555,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2894+43.9366 20260325.4555 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:07.04 +43:56:01.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.45 21:44:16.56 +43:16:44.0
90.57181 -7.52854 galactic Cyg Second-epoch detections are separated by 2.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.0747+43.2732 | 21:44:16.56 +43:16:44.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.0747+43.2732,2461124.9555,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.0747+43.2732 20260325.4555 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:16.56 +43:16:44.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.79 21:00:18.71 +47:17:58.3
87.91673 0.76317 galactic Cyg Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:18.71 +47:17:58.3 (user input) | T | P | (position from user input) J-Ks=0.510+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:18.71 +47:17:58.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.70 21:01:59.88 +47:36:05.9
88.33187 0.74841 galactic Cyg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:59.88 +47:36:05.9 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:59.88 +47:36:05.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.57 21:00:49.27 +47:13:06.5
87.91266 0.64476 galactic Cyg Second-epoch detections are separated by 0.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2134+47.2161 | 21:00:49.17 +47:13:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: C 1960RA......6..301M CGCS 5088 J-Ks=1.302+/-0.027 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2134+47.2161,2461124.9555,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2134+47.2161 20260325.4555 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:49.27 +47:13:06.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.33 21:01:30.61 +46:16:02.9
87.27618 -0.07165 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3770+46.2677 | 21:01:30.61 +46:16:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.825+/-0.050 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3770+46.2677,2461124.9555,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3770+46.2677 20260325.4555 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:30.61 +46:16:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.68 21:01:35.28 +47:24:12.4
88.13742 0.66923 galactic Cyg Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4051+47.4028 | 21:01:35.28 +47:24:12.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.336+/-0.036 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4051+47.4028,2461124.9555,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4051+47.4028 20260325.4555 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:35.28 +47:24:12.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.29 21:43:21.11 +43:32:30.7
90.61774 -7.21991 galactic Cyg Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8341+43.5513 | 21:43:21.11 +43:32:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.931+/-0.025 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8341+43.5513,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8341+43.5513 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:21.11 +43:32:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.26 21:46:57.85 +44:28:25.6
91.72601 -6.93579 galactic Cyg Second-epoch detections are separated by 1.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.7407+44.4741 | 21:46:57.78 +44:28:27.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.267+/-0.035 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.7407+44.4741,2461124.9555,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.7407+44.4741 20260325.4555 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:57.85 +44:28:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163632729356659968,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163632729356659968 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:22.16 +46:19:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163656781173423488,2461124.9555,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163656781173423488 20260325.4555 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:58.11 +46:44:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.93 21:01:45.71 +47:20:23.6
88.10920 0.60512 galactic Cyg Second-epoch detections are separated by 1.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4402+47.3424 | 21:01:45.71 +47:20:23.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.504+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4402+47.3424,2461124.9555,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4402+47.3424 20260325.4555 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:45.71 +47:20:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:44:37.00 +43:37:40.5
90.84907 -7.30482 galactic Cyg Second-epoch detections are separated by 1.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:37.00 +43:37:40.5 (user input) | T | P | (position from user input) J-Ks=0.834+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:37.00 +43:37:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.60 22:12:11.13 +49:35:54.6
98.29201 -5.50015 galactic Lac Second-epoch detections are separated by 2.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976703314396476800 | 22:12:11.18 +49:35:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.816+/-0.029 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976703314396476800,2461124.9555,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976703314396476800 20260325.4555 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:11.13 +49:35:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.11 21:01:40.40 +46:34:08.0
87.52092 0.10652 galactic Cyg Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4191+46.5719 | 21:01:40.40 +46:34:08.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: B:e 1973A&AS....9..183W UHA 119 J-Ks=0.346+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4191+46.5719,2461124.9555,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4191+46.5719 20260325.4555 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:40.40 +46:34:08.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210122.05+470606.4,2461124.9555,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210122.05+470606.4 20260325.4555 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:21.15 +47:05:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.34 21:02:53.33 +47:14:25.7
88.16143 0.39613 galactic Cyg Second-epoch detections are separated by 3.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7302+47.2414 | 21:02:53.33 +47:14:25.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7302+47.2414,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7302+47.2414 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:53.33 +47:14:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163880359978956416,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163880359978956416 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:15.69 +47:12:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.14 21:00:21.50 +47:29:48.5
88.07047 0.88706 galactic Cyg Second-epoch detections are separated by 0.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163946949154010368 | 21:00:21.36 +47:29:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.276+/-0.027 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163946949154010368,2461124.9555,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163946949154010368 20260325.4555 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:21.50 +47:29:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163867505130913024,2461124.9555,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163867505130913024 20260325.4555 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:26.69 +47:04:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.00 21:00:36.25 +46:12:48.1
87.13215 0.01035 galactic Cyg Second-epoch detections are separated by 0.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1511+46.2135 | 21:00:36.25 +46:12:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.151+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1511+46.2135,2461124.9555,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1511+46.2135 20260325.4555 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:36.25 +46:12:48.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.52 21:01:38.56 +47:22:15.5
88.11917 0.64082 galactic Cyg Second-epoch detections are separated by 0.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4104+47.3768 | 21:01:38.56 +47:22:15.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.524+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4104+47.3768,2461124.9555,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4104+47.3768 20260325.4555 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:38.56 +47:22:15.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.62 21:02:22.22 +42:50:31.9
84.80853 -2.45294 galactic Cyg Second-epoch detections are separated by 1.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:22.22 +42:50:31.9 (user input) | T | P | (position from user input) J-Ks=0.615+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:22.22 +42:50:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:03:16.95 +47:18:56.9
88.26210 0.39631 galactic Cyg Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.8216+47.3203 | 21:03:16.95 +47:18:56.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.402+/-0.029 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.8216+47.3203,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.8216+47.3203 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:16.95 +47:18:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163472338093467520,2461124.9555,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163472338093467520 20260325.4555 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:26.14 +45:46:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163634275547427456,2461124.9555,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163634275547427456 20260325.4555 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:11.44 +46:27:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.39 21:00:39.36 +47:14:04.7
87.90633 0.67650 galactic Cyg Second-epoch detections are separated by 0.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163892798204145920 | 21:00:39.31 +47:14:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.355+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163892798204145920,2461124.9555,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163892798204145920 20260325.4555 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:39.36 +47:14:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.48 21:00:12.04 +47:54:15.9
88.36006 1.17519 galactic Cyg Second-epoch detections are separated by 2.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:12.04 +47:54:15.9 (user input) | T | P | (position from user input) J-Ks=0.886+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:12.04 +47:54:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163485257355382656,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163485257355382656 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:33.79 +46:02:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.09 21:00:50.61 +47:55:23.3
88.44508 1.10645 galactic Cyg Second-epoch detections are separated by 2.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2255+47.9221 | 21:00:50.61 +47:55:23.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.329+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2255+47.9221,2461124.9555,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2255+47.9221 20260325.4555 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:50.61 +47:55:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 10.92 21:00:52.66 +47:40:07.2
88.25749 0.93437 galactic Cyg Second-epoch detections are separated by 0.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2243+47.6747 | 21:00:52.65 +47:40:06.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.838+/- (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2243+47.6747,2461124.9555,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2243+47.6747 20260325.4555 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:52.66 +47:40:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.30 21:03:12.89 +47:51:12.9
88.65617 0.76245 galactic Cyg Second-epoch detections are separated by 1.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.8035+47.8538 | 21:03:12.89 +47:51:12.9 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.552+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.8035+47.8538,2461124.9555,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.8035+47.8538 20260325.4555 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:12.89 +47:51:12.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.57 21:02:56.12 +47:08:25.4
88.09186 0.32375 galactic Cyg Second-epoch detections are separated by 0.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7506+47.1360 | 21:02:59.22 +47:07:54.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7506+47.1360,2461124.9555,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7506+47.1360 20260325.4555 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:56.12 +47:08:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J210026.96+471654.5,2461124.9555,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J210026.96+471654.5 20260325.4555 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:26.99 +47:16:52.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163479244401126016,2461124.9555,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163479244401126016 20260325.4555 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:46.70 +45:54:21.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.84 21:01:15.94 +47:57:35.1
88.51925 1.07746 galactic Cyg Second-epoch detections are separated by 0.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3111+47.9614 | 21:01:15.94 +47:57:35.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.374+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3111+47.9614,2461124.9555,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3111+47.9614 20260325.4555 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:15.94 +47:57:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.13 21:44:48.67 +43:42:11.4
90.92546 -7.27078 galactic Cyg Second-epoch detections are separated by 1.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.2000+43.7035 | 21:44:48.67 +43:42:11.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.007+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.2000+43.7035,2461124.9555,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2000+43.7035 20260325.4555 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:48.67 +43:42:11.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163648191238157952,2461124.9555,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163648191238157952 20260325.4555 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:19.24 +46:32:51.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214155.36+424507.3,2461124.9555,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214155.36+424507.3 20260325.4555 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:55.36 +42:45:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210232.96+470544.6,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210232.96+470544.6 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:34.58 +47:05:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.96 21:03:20.15 +47:52:05.2
88.68052 0.75696 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2165414414907361024 | 21:03:19.91 +47:52:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165414414907361024,2461124.9555,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165414414907361024 20260325.4555 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:20.15 +47:52:05.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.27 21:01:06.83 +45:55:39.0
86.97552 -0.24460 galactic Cyg Second-epoch detections are separated by 1.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:06.83 +45:55:39.0 (user input) | T | P | (position from user input) J-Ks=0.894+/-0.036 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:06.83 +45:55:39.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:44:41.65 +43:53:38.5
91.03487 -7.11237 galactic Cyg Second-epoch detections are separated by 0.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1864+43.8936 | 21:44:41.65 +43:53:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.984+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1864+43.8936,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1864+43.8936 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:41.65 +43:53:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.09 21:00:56.64 +47:45:39.5
88.33426 0.98685 galactic Cyg Second-epoch detections are separated by 0.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:56.64 +47:45:39.5 (user input) | T | P | (position from user input) J-Ks=1.021+/-0.037 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:56.64 +47:45:39.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.98 21:41:07.22 +42:35:09.6
89.67293 -7.66947 galactic Cyg Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2859+42.5863 | 21:41:07.19 +42:35:10.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5) J-Ks=1.239+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2859+42.5863,2461124.9555,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2859+42.5863 20260325.4555 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:07.22 +42:35:09.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.77 22:09:01.64 +49:22:14.8
97.73921 -5.39008 galactic Lac Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.2638+49.3650 | 22:09:01.77 +49:22:18.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2638+49.3650,2461124.9555,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2638+49.3650 20260325.4555 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:01.64 +49:22:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.47 21:01:17.60 +46:44:42.6
87.61013 0.27195 galactic Cyg Second-epoch detections are separated by 3.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3141+46.7466 | 21:01:17.60 +46:44:42.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.466+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3141+46.7466,2461124.9555,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3141+46.7466 20260325.4555 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:17.60 +46:44:42.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.51 21:47:17.98 +44:02:39.3
91.49258 -7.30246 galactic Cyg Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:17.98 +44:02:39.3 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:17.98 +44:02:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.47 21:01:57.15 +47:04:09.8
87.92781 0.40185 galactic Cyg Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4928+47.0641 | 21:01:57.15 +47:04:09.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.828+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4928+47.0641,2461124.9555,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4928+47.0641 20260325.4555 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:57.15 +47:04:09.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:31.27 +46:49:47.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.92 21:03:44.81 +47:54:42.4
88.75897 0.73461 galactic Cyg Second-epoch detections are separated by 1.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.9346+47.9148 | 21:03:44.68 +47:54:43.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.932+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.9346+47.9148,2461124.9555,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.9346+47.9148 20260325.4555 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:44.81 +47:54:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163644961423500800,2461124.9555,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163644961423500800 20260325.4555 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:27.96 +46:42:00.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:40:11.37 +42:48:51.6
89.69685 -7.38518 galactic Cyg Second-epoch detections are separated by 1.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:11.37 +42:48:51.6 (user input) | T | P | (position from user input) J-Ks=0.238+/-0.032 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:11.37 +42:48:51.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:01:54.84 +46:14:13.6
87.29958 -0.14410 galactic Cyg Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4756+46.2430 | 21:01:54.84 +46:14:13.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.362+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4756+46.2430,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4756+46.2430 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:54.84 +46:14:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.39 22:11:04.37 +49:35:08.6
98.13633 -5.40709 galactic Lac Second-epoch detections are separated by 1.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.7823+49.5870 | 22:11:04.28 +49:35:11.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.7823+49.5870,2461124.9555,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.7823+49.5870 20260325.4555 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:04.37 +49:35:08.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.17 21:01:46.97 +47:25:14.5
88.17216 0.65591 galactic Cyg Second-epoch detections are separated by 2.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4405+47.4221 | 21:01:46.97 +47:25:14.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4405+47.4221,2461124.9555,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4405+47.4221 20260325.4555 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:46.97 +47:25:14.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165428231820175360,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165428231820175360 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:25.45 +47:57:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.40 21:00:23.24 +46:57:54.6
87.67342 0.53345 galactic Cyg Second-epoch detections are separated by 0.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0973+46.9603 | 21:00:23.23 +46:57:55.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0973+46.9603,2461124.9555,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0973+46.9603 20260325.4555 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:23.24 +46:57:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163482474216663168,2461124.9555,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163482474216663168 20260325.4555 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:48.44 +46:02:22.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.52 21:42:28.79 +42:49:49.7
90.02508 -7.65116 galactic Cyg Second-epoch detections are separated by 0.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:28.79 +42:49:49.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.414+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:28.79 +42:49:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.42 21:01:56.76 +46:26:30.0
87.45657 -0.01284 galactic Cyg Second-epoch detections are separated by 1.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4865+46.4440 | 21:01:56.76 +46:26:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4865+46.4440,2461124.9555,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4865+46.4440 20260325.4555 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:56.76 +46:26:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:52.14 +47:37:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.34 21:02:58.76 +47:52:40.4
88.64808 0.80812 galactic Cyg Second-epoch detections are separated by 1.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7464+47.8827 | 21:02:58.76 +47:52:40.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.682+/-0.026 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7464+47.8827,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7464+47.8827 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:58.76 +47:52:40.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.22 21:45:40.24 +44:01:21.8
91.25372 -7.12917 galactic Cyg Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:40.24 +44:01:21.8 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:40.24 +44:01:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.34 21:00:44.06 +47:50:17.9
88.36920 1.06430 galactic Cyg Second-epoch detections are separated by 1.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1778+47.8374 | 21:00:44.06 +47:50:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.257+/-0.032 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1778+47.8374,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1778+47.8374 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:44.06 +47:50:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.58 21:01:06.42 +47:49:44.7
88.40351 1.01120 galactic Cyg Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2766+47.8294 | 21:01:06.40 +47:49:46.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2766+47.8294,2461124.9555,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2766+47.8294 20260325.4555 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:06.42 +47:49:44.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.12 21:02:14.94 +46:25:35.7
87.47984 -0.06194 galactic Cyg Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5620+46.4269 | 21:02:14.94 +46:25:35.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.702+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5620+46.4269,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5620+46.4269 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:14.94 +46:25:35.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.04 21:45:21.29 +43:25:05.6
90.81343 -7.55105 galactic Cyg Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972908139547344384 | 21:45:21.26 +43:25:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.187+/-0.023 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972908139547344384,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972908139547344384 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:21.29 +43:25:05.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.24 21:00:59.22 +47:53:10.6
88.43323 1.06406 galactic Cyg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2482+47.8853 | 21:00:59.22 +47:53:10.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2482+47.8853,2461124.9555,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2482+47.8853 20260325.4555 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:59.22 +47:53:10.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J210115.76+472230.9,2461124.9555,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J210115.76+472230.9 20260325.4555 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:15.87 +47:22:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.40 21:03:15.41 +47:54:39.8
88.70378 0.79541 galactic Cyg Second-epoch detections are separated by 2.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:15.41 +47:54:39.8 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.029 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:15.41 +47:54:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.27 21:46:26.80 +43:50:35.2
91.24333 -7.35648 galactic Cyg Second-epoch detections are separated by 0.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1973020603272055680 | 21:46:28.46 +43:51:16.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973020603272055680,2461124.9555,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973020603272055680 20260325.4555 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:26.80 +43:50:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163635649933655808,2461124.9555,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163635649933655808 20260325.4555 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:29.37 +46:29:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.90 21:00:47.85 +47:07:24.2
87.83850 0.58510 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:47.85 +47:07:24.2 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:47.85 +47:07:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.01 21:02:07.28 +46:39:22.5
87.63733 0.10666 galactic Cyg Second-epoch detections are separated by 0.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5291+46.6525 | 21:02:07.28 +46:39:22.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.147+/-0.036 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5291+46.6525,2461124.9555,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5291+46.6525 20260325.4555 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:07.28 +46:39:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J220720.25+485047.8,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220720.25+485047.8 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:19.91 +48:50:45.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.12 21:47:08.06 +44:35:10.4
91.82249 -6.86954 galactic Cyg Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:08.06 +44:35:10.4 (user input) | T | P | (position from user input) J-Ks=0.898+/-0.063 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:08.06 +44:35:10.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:01:19.74 +46:38:16.3
87.53359 0.19649 galactic Cyg Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3359+46.6452 | 21:01:19.74 +46:38:16.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.397+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3359+46.6452,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3359+46.6452 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:19.74 +46:38:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.09 21:44:37.68 +43:49:23.1
90.97909 -7.15834 galactic Cyg Second-epoch detections are separated by 1.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:37.68 +43:49:23.1 (user input) | T | P | (position from user input) J-Ks=0.765+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:37.68 +43:49:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:03:25.89 +47:38:60.0
88.52837 0.59984 galactic Cyg Second-epoch detections are separated by 0.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.8614+47.6571 | 21:03:25.86 +47:39:01.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.958+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.8614+47.6571,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.8614+47.6571 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:25.89 +47:38:60.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J210007.73+475001.5,2461124.9555,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J210007.73+475001.5 20260325.4555 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:07.72 +47:50:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163627850272734464,2461124.9555,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163627850272734464 20260325.4555 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:29.04 +46:11:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163947155312485632,2461124.9555,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163947155312485632 20260325.4555 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:24.64 +47:32:02.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.18 21:01:47.69 +42:44:55.1
84.66840 -2.43565 galactic Cyg Second-epoch detections are separated by 2.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4352+42.7521 | 21:01:47.69 +42:44:55.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.705+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4352+42.7521,2461124.9555,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4352+42.7521 20260325.4555 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:47.69 +42:44:55.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.29 21:43:55.89 +44:15:44.6
91.17284 -6.74401 galactic Cyg Second-epoch detections are separated by 3.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.9816+44.2532 | 21:43:55.89 +44:15:44.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.357+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.9816+44.2532,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.9816+44.2532 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:55.89 +44:15:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.28 21:45:47.46 +43:43:38.4
91.07679 -7.36774 galactic Cyg Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.4465+43.7251 | 21:45:47.46 +43:43:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.505+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.4465+43.7251,2461124.9555,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.4465+43.7251 20260325.4555 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:47.46 +43:43:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:01:07.74 +47:34:38.7
88.21684 0.84235 galactic Cyg Second-epoch detections are separated by 0.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2984+47.5811 | 21:01:11.24 +47:34:37.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.147+/-0.037 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2984+47.5811,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2984+47.5811 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:07.74 +47:34:38.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973511049876940544,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973511049876940544 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:36.69 +44:56:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.09 21:02:12.13 +47:16:49.6
88.11406 0.50983 galactic Cyg Second-epoch detections are separated by 0.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163884410118603520 | 21:02:12.08 +47:16:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.084+/-0.032 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163884410118603520,2461124.9555,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163884410118603520 20260325.4555 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:12.13 +47:16:49.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.05 21:58:44.28 +46:55:38.0
94.88858 -6.32432 galactic Cyg Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6843+46.9278 | 21:58:44.25 +46:55:40.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.219+/-0.029 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6843+46.9278,2461124.9555,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6843+46.9278 20260325.4555 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:44.28 +46:55:38.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.70 21:00:11.76 +47:53:24.2
88.34872 1.16634 galactic Cyg Second-epoch detections are separated by 1.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0593+47.8834 | 21:00:11.76 +47:53:24.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0593+47.8834,2461124.9555,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0593+47.8834 20260325.4555 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:11.76 +47:53:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.51 21:02:43.22 +46:59:46.5
87.95978 0.25541 galactic Cyg Second-epoch detections are separated by 1.7" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6870+46.9908 | 21:02:43.22 +46:59:46.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.399+/-0.061 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6870+46.9908,2461124.9555,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6870+46.9908 20260325.4555 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:43.22 +46:59:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165403767697761152,2461124.9555,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165403767697761152 20260325.4555 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:42.43 +47:50:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.63 21:01:24.45 +46:22:15.9
87.34223 0.01012 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3445+46.3611 | 21:01:24.42 +46:22:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.463+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3445+46.3611,2461124.9555,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3445+46.3611 20260325.4555 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:24.45 +46:22:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.33 21:01:01.46 +47:51:41.2
88.41869 1.04298 galactic Cyg Second-epoch detections are separated by 0.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2527+47.8630 | 21:01:01.50 +47:51:41.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2527+47.8630,2461124.9555,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2527+47.8630 20260325.4555 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:01.46 +47:51:41.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:46.35 +47:54:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.04 21:00:36.27 +46:25:02.5
87.28567 0.14470 galactic Cyg Second-epoch detections are separated by 0.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1510+46.4170 | 21:00:36.27 +46:25:02.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.771+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1510+46.4170,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1510+46.4170 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:36.27 +46:25:02.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.57 21:00:16.88 +47:12:34.7
87.84563 0.70792 galactic Cyg Second-epoch detections are separated by 1.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0689+47.1986 | 21:00:16.88 +47:12:34.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.988+/-0.038 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0689+47.1986,2461124.9555,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0689+47.1986 20260325.4555 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:16.88 +47:12:34.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.39 21:01:36.59 +46:43:18.2
87.62837 0.21575 galactic Cyg Second-epoch detections are separated by 2.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3943+46.7141 | 21:01:36.58 +46:43:20.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.288+/-0.033 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3943+46.7141,2461124.9555,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3943+46.7141 20260325.4555 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:36.59 +46:43:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.27 21:04:04.48 +47:50:17.6
88.74078 0.64460 galactic Cyg Second-epoch detections are separated by 5.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.0255+47.8393 | 21:04:06.12 +47:50:21.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.0255+47.8393,2461124.9555,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.0255+47.8393 20260325.4555 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:04.48 +47:50:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5931073,2461124.9555,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5931073 20260325.4555 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:01.30 +44:39:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.59 21:00:35.54 +47:02:37.3
87.75554 0.55886 galactic Cyg Second-epoch detections are separated by 0.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:35.54 +47:02:37.3 (user input) | T | P | (position from user input) J-Ks=0.450+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:35.54 +47:02:37.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.55 21:02:27.46 +47:00:00.9
87.93305 0.29157 galactic Cyg Second-epoch detections are separated by 1.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6248+46.9943 | 21:02:27.46 +47:00:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.739+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6248+46.9943,2461124.9555,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6248+46.9943 20260325.4555 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:27.46 +47:00:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:12.83 +44:01:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.65 21:01:53.32 +42:46:25.5
84.69866 -2.43198 galactic Cyg Second-epoch detections are separated by 1.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:53.32 +42:46:25.5 (user input) | T | P | (position from user input) J-Ks=0.507+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:53.32 +42:46:25.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.36 21:02:15.11 +47:36:31.5
88.36554 0.72106 galactic Cyg Second-epoch detections are separated by 2.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5652+47.6124 | 21:02:15.11 +47:36:31.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.271+/-0.033 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5652+47.6124,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5652+47.6124 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:15.11 +47:36:31.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.49 21:01:07.81 +47:25:27.1
88.10184 0.74109 galactic Cyg Second-epoch detections are separated by 2.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2789+47.4216 | 21:01:07.81 +47:25:27.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.135+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2789+47.4216,2461124.9555,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2789+47.4216 20260325.4555 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:07.81 +47:25:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.58 21:01:45.94 +47:23:15.0
88.14534 0.63613 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4338+47.3980 | 21:01:45.94 +47:23:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.377+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4338+47.3980,2461124.9555,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4338+47.3980 20260325.4555 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:45.94 +47:23:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163627781553260160,2461124.9555,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163627781553260160 20260325.4555 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:33.41 +46:11:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.54 21:01:55.93 +46:00:20.1
87.12811 -0.29970 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:55.93 +46:00:20.1 (user input) | T | P | (position from user input) J-Ks=0.883+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:55.93 +46:00:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J215037.79+430852.0,2461124.9555,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215037.79+430852.0 20260325.4555 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:37.88 +43:08:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.54 21:03:43.22 +47:52:40.9
88.73084 0.71544 galactic Cyg Second-epoch detections are separated by 0.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.9238+47.8660 | 21:03:43.22 +47:52:40.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=12.118+/- (unrealisitic color!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.9238+47.8660,2461124.9555,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.9238+47.8660 20260325.4555 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:43.22 +47:52:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:00:35.49 +47:06:30.4
87.80417 0.60162 galactic Cyg Second-epoch detections are separated by 0.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163868020526987136 | 21:00:35.21 +47:07:09.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.756+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163868020526987136,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163868020526987136 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:35.49 +47:06:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.36 21:01:51.62 +47:43:23.7
88.40770 0.84627 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2165410119940077568 | 21:01:51.65 +47:43:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.293+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165410119940077568,2461124.9555,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165410119940077568 20260325.4555 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:51.62 +47:43:23.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972969372904277888,2461124.9555,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972969372904277888 20260325.4555 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:14.65 +43:36:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.12 21:01:37.03 +43:27:40.2
85.18217 -1.94050 galactic Cyg Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:37.03 +43:27:40.2 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:37.03 +43:27:40.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2152496+463713,2461124.9555,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2152496+463713 20260325.4555 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:49.64 +46:37:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213617.94+430244.2,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213617.94+430244.2 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:17.87 +43:02:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.93 21:00:26.73 +47:46:46.9
88.29315 1.06220 galactic Cyg Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1092+47.7826 | 21:00:26.73 +47:46:46.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.436+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1092+47.7826,2461124.9555,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1092+47.7826 20260325.4555 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:26.73 +47:46:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.07 21:01:44.25 +45:45:58.0
86.92613 -0.43275 galactic Cyg Second-epoch detections are separated by 1.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4443+45.7558 | 21:01:44.25 +45:45:58.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.396+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4443+45.7558,2461124.9555,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4443+45.7558 20260325.4555 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:44.25 +45:45:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.12 21:01:09.22 +46:18:42.9
87.26887 0.00394 galactic Cyg Second-epoch detections are separated by 0.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2883+46.3121 | 21:01:09.22 +46:18:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.321+/-0.035 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2883+46.3121,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2883+46.3121 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:09.22 +46:18:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5840473,2461124.9555,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5840473 20260325.4555 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:14.83 +47:06:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.35 21:01:19.61 +47:16:27.8
88.01130 0.61717 galactic Cyg Second-epoch detections are separated by 6.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163882249764603776 | 21:01:19.66 +47:16:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163882249764603776,2461124.9555,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163882249764603776 20260325.4555 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:19.61 +47:16:27.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.65 21:01:34.86 +43:35:54.5
85.28097 -1.84487 galactic Cyg Second-epoch detections are separated by 1.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3947+43.5989 | 21:01:34.86 +43:35:54.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.010+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3947+43.5989,2461124.9555,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3947+43.5989 20260325.4555 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:34.86 +43:35:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:27.49 +43:26:11.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.73 21:02:41.13 +47:17:01.0
88.17079 0.45057 galactic Cyg Second-epoch detections are separated by 1.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6710+47.2841 | 21:02:41.13 +47:17:01.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.462+/-0.040 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6710+47.2841,2461124.9555,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6710+47.2841 20260325.4555 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:41.13 +47:17:01.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:25.41 +47:47:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.55 21:01:08.50 +47:39:27.5
88.27853 0.89369 galactic Cyg Second-epoch detections are separated by 0.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163953954227538176 | 21:01:08.46 +47:39:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163953954227538176,2461124.9555,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163953954227538176 20260325.4555 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:08.50 +47:39:27.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972864124721766144,2461124.9555,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972864124721766144 20260325.4555 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:28.69 +42:50:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.81 21:01:11.25 +47:34:36.1
88.22281 0.83446 galactic Cyg Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2984+47.5811 | 21:01:11.24 +47:34:37.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.104+/-0.038 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2984+47.5811,2461124.9555,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2984+47.5811 20260325.4555 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:11.25 +47:34:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.19 21:00:48.90 +46:26:08.0
87.32326 0.12941 galactic Cyg Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:48.90 +46:26:08.0 (user input) | T | P | (position from user input) J-Ks=0.258+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:48.90 +46:26:08.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.70 21:02:52.62 +47:33:34.2
88.39862 0.60951 galactic Cyg Second-epoch detections are separated by 2.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7230+47.5621 | 21:02:52.62 +47:33:34.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.202+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7230+47.5621,2461124.9555,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7230+47.5621 20260325.4555 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:52.62 +47:33:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.60 21:00:49.47 +47:13:47.2
87.92153 0.65178 galactic Cyg Second-epoch detections are separated by 0.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2134+47.2161 | 21:00:49.17 +47:13:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: C 1960RA......6..301M CGCS 5088 J-Ks=0.359+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2134+47.2161,2461124.9555,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2134+47.2161 20260325.4555 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:49.47 +47:13:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.13 21:02:49.04 +47:01:18.2
87.98980 0.25995 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7029+47.0257 | 21:02:49.04 +47:01:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.266+/-0.052 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7029+47.0257,2461124.9555,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7029+47.0257 20260325.4555 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:49.04 +47:01:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210209.95+462428.1,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210209.95+462428.1 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:10.08 +46:24:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.79 21:01:22.56 +47:30:32.2
88.19293 0.76584 galactic Cyg Second-epoch detections are separated by 0.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163905403918737920 | 21:01:22.39 +47:30:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163905403918737920,2461124.9555,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163905403918737920 20260325.4555 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:22.56 +47:30:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.80 21:01:42.77 +47:15:05.6
88.03745 0.55293 galactic Cyg Second-epoch detections are separated by 0.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163881528210161792 | 21:01:42.71 +47:15:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.354+/-0.028 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163881528210161792,2461124.9555,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163881528210161792 20260325.4555 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:42.77 +47:15:05.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:02:09.60 +46:09:28.1
87.26834 -0.22851 galactic Cyg Second-epoch detections are separated by 1.7" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:09.60 +46:09:28.1 (user input) | T | P | (position from user input) J-Ks=0.866+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:09.60 +46:09:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.31 21:00:28.29 +46:48:39.2
87.56675 0.42106 galactic Cyg Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:28.29 +46:48:39.2 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:28.29 +46:48:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.08 21:02:05.91 +46:40:05.4
87.64366 0.11749 galactic Cyg Second-epoch detections are separated by 0.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5205+46.6646 | 21:02:05.91 +46:40:05.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.368+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5205+46.6646,2461124.9555,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5205+46.6646 20260325.4555 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:05.91 +46:40:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163639047230392832,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163639047230392832 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:36.53 +46:30:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163481546503853184,2461124.9555,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163481546503853184 20260325.4555 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:45.06 +45:56:35.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.60 21:02:47.34 +43:03:31.5
85.02166 -2.36680 galactic Cyg Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:47.34 +43:03:31.5 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:47.34 +43:03:31.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.04 21:01:01.67 +46:30:17.8
87.39958 0.14762 galactic Cyg Second-epoch detections are separated by 1.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2647+46.5144 | 21:01:03.55 +46:30:51.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.458+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2647+46.5144,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2647+46.5144 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:01.67 +46:30:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.37 21:01:07.73 +46:02:12.6
87.05938 -0.17439 galactic Cyg Second-epoch detections are separated by 1.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:07.73 +46:02:12.6 (user input) | T | P | (position from user input) J-Ks=0.929+/-0.032 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:07.73 +46:02:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.56 21:02:57.65 +43:48:19.2
85.60129 -1.89473 galactic Cyg Second-epoch detections are separated by 2.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7382+43.8023 | 21:02:57.65 +43:48:19.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.533+/-0.077 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7382+43.8023,2461124.9555,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7382+43.8023 20260325.4555 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:57.65 +43:48:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.31 21:01:12.66 +47:53:16.1
88.45916 1.03685 galactic Cyg Second-epoch detections are separated by 1.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:12.66 +47:53:16.1 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:12.66 +47:53:16.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163645816098547840,2461124.9555,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163645816098547840 20260325.4555 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:49.12 +46:27:02.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163971550726908160,2461124.9555,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163971550726908160 20260325.4555 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:21.45 +47:50:50.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973030017840497152,2461124.9555,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973030017840497152 20260325.4555 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:31.69 +43:57:33.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.52 21:00:24.71 +46:51:21.6
87.59399 0.45844 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:24.71 +46:51:21.6 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:24.71 +46:51:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2137160+435238,2461124.9555,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2137160+435238 20260325.4555 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:14.43 +43:52:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.03 21:00:58.49 +47:00:10.6
87.76786 0.48298 galactic Cyg Second-epoch detections are separated by 0.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2369+47.0079 | 21:00:58.49 +47:00:10.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.419+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2369+47.0079,2461124.9555,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2369+47.0079 20260325.4555 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:58.49 +47:00:10.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163678599608596736,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163678599608596736 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:02.74 +47:01:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.63 21:00:51.95 +47:44:30.1
88.31110 0.98402 galactic Cyg Second-epoch detections are separated by 1.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:51.95 +47:44:30.1 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:51.95 +47:44:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.51 21:00:19.63 +47:39:08.7
88.18420 0.99342 galactic Cyg Second-epoch detections are separated by 1.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2163951759517479808 | 21:00:19.63 +47:39:08.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.387+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2163951759517479808,2461124.9555,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2163951759517479808 20260325.4555 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:19.63 +47:39:08.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.11 21:02:25.44 +47:00:50.4
87.93954 0.30499 galactic Cyg Second-epoch detections are separated by 0.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6056+47.0153 | 21:02:27.73 +47:00:59.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.512+/-0.046 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6056+47.0153,2461124.9555,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6056+47.0153 20260325.4555 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:25.44 +47:00:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.07 21:42:13.13 +43:16:50.4
90.28831 -7.28126 galactic Cyg Second-epoch detections are separated by 1.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:13.13 +43:16:50.4 (user input) | T | P | (position from user input) J-Ks=2.909+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:13.13 +43:16:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163882627721785856,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163882627721785856 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:33.44 +47:18:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.61 21:00:16.39 +47:15:21.2
87.87955 0.73940 galactic Cyg Second-epoch detections are separated by 3.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0652+47.2568 | 21:00:16.39 +47:15:21.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=11.948+/- (unrealisitic color!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0652+47.2568,2461124.9555,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0652+47.2568 20260325.4555 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:16.39 +47:15:21.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:02:50.98 +47:39:38.5
88.47122 0.68015 galactic Cyg Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:50.98 +47:39:38.5 (user input) | T | P | (position from user input) J-Ks=0.450+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:50.98 +47:39:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966921749712900352,2461124.9555,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966921749712900352 20260325.4555 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:11.13 +42:55:31.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.19 21:00:52.61 +47:33:02.8
88.16875 0.85675 galactic Cyg Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2278+47.5405 | 21:00:52.61 +47:33:02.8 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.351+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2278+47.5405,2461124.9555,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2278+47.5405 20260325.4555 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:52.61 +47:33:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.56 21:02:33.13 +41:55:25.8
84.14181 -3.08622 galactic Cyg Second-epoch detections are separated by 2.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6376+41.9261 | 21:02:33.13 +41:55:25.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6376+41.9261,2461124.9555,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6376+41.9261 20260325.4555 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:33.13 +41:55:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:01:31.06 +46:50:45.4
87.71115 0.30971 galactic Cyg Second-epoch detections are separated by 1.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3808+46.8435 | 21:01:31.06 +46:50:45.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3808+46.8435,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3808+46.8435 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:31.06 +46:50:45.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214328.55+424819.2,2461124.9555,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214328.55+424819.2 20260325.4555 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:28.59 +42:48:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.52 21:00:28.66 +46:35:37.0
87.40392 0.27720 galactic Cyg Second-epoch detections are separated by 0.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1195+46.5938 | 21:00:28.66 +46:35:37.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.412+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1195+46.5938,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1195+46.5938 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:28.66 +46:35:37.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.54 21:43:35.41 +43:40:39.7
90.74037 -7.14569 galactic Cyg Second-epoch detections are separated by 3.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:35.41 +43:40:39.7 (user input) | T | P | (position from user input) J-Ks=1.060+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:35.41 +43:40:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.83 21:02:29.34 +47:42:30.7
88.46673 0.75730 galactic Cyg Second-epoch detections are separated by 0.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6040+47.7105 | 21:02:29.34 +47:42:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.288+/-0.044 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6040+47.7105,2461124.9555,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6040+47.7105 20260325.4555 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:29.34 +47:42:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163893725917139200,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163893725917139200 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:48.71 +47:19:28.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.38 21:01:08.44 +45:39:36.1
86.77766 -0.42464 galactic Cyg Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2987+45.6626 | 21:01:08.44 +45:39:36.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.754+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2987+45.6626,2461124.9555,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2987+45.6626 20260325.4555 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:08.44 +45:39:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.22 21:44:30.99 +42:43:17.8
90.23736 -7.97873 galactic Cyg Second-epoch detections are separated by 1.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1378+42.7293 | 21:44:30.99 +42:43:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.280+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1378+42.7293,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1378+42.7293 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:30.99 +42:43:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.11 21:01:44.34 +47:03:38.9
87.89732 0.42343 galactic Cyg Second-epoch detections are separated by 0.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4218+47.0531 | 21:01:44.34 +47:03:38.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.163+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4218+47.0531,2461124.9555,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4218+47.0531 20260325.4555 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:44.34 +47:03:38.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.22 21:02:05.80 +43:40:49.4
85.40418 -1.86069 galactic Cyg Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:05.80 +43:40:49.4 (user input) | T | P | (position from user input) J-Ks=0.694+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:05.80 +43:40:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.93 21:00:39.39 +47:48:27.1
88.33744 1.05385 galactic Cyg Second-epoch detections are separated by 0.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1572+47.8006 | 21:00:39.39 +47:48:27.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.253+/-0.035 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1572+47.8006,2461124.9555,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1572+47.8006 20260325.4555 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:39.39 +47:48:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163904583594770048,2461124.9555,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163904583594770048 20260325.4555 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:53.80 +47:35:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.67 21:01:03.33 +47:06:17.9
87.85361 0.53996 galactic Cyg Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2608+47.1063 | 21:01:03.33 +47:06:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2608+47.1063,2461124.9555,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2608+47.1063 20260325.4555 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:03.33 +47:06:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.57 21:00:56.50 +46:41:10.3
87.52604 0.27831 galactic Cyg Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:56.50 +46:41:10.3 (user input) | T | P | (position from user input) J-Ks=0.725+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:56.50 +46:41:10.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.55 21:02:19.26 +47:41:50.1
88.43954 0.77099 galactic Cyg Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5755+47.7025 | 21:02:19.18 +47:41:51.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.014+/-0.029 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5755+47.7025,2461124.9555,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5755+47.7025 20260325.4555 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:19.26 +47:41:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.41 21:43:38.89 +43:37:42.6
90.71585 -7.18971 galactic Cyg Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:38.89 +43:37:42.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.454+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:38.89 +43:37:42.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210156.84+470259.8,2461124.9555,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210156.84+470259.8 20260325.4555 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:55.27 +47:03:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.37 21:03:52.08 +42:49:39.7
84.98014 -2.66789 galactic Cyg Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.9804+42.8298 | 21:03:51.92 +42:49:40.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.447+/-0.029 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.9804+42.8298,2461124.9555,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.9804+42.8298 20260325.4555 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:52.08 +42:49:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.04 21:02:23.53 +42:21:57.0
84.45383 -2.77135 galactic Cyg Second-epoch detections are separated by 0.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5973+42.3659 | 21:02:23.37 +42:21:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.425+/-0.049 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5973+42.3659,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5973+42.3659 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:23.53 +42:21:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163631114448954624,2461124.9555,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163631114448954624 20260325.4555 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:45.40 +46:21:17.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J210036.86+471235.3,2461124.9555,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J210036.86+471235.3 20260325.4555 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:36.95 +47:12:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.08 21:00:24.33 +47:43:19.3
88.24530 1.02930 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2163958047344230400 | 21:00:24.33 +47:43:19.3 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.354+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2163958047344230400,2461124.9555,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2163958047344230400 20260325.4555 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:24.33 +47:43:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.88 21:01:39.88 +45:56:16.0
87.04651 -0.30971 galactic Cyg Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4159+45.9379 | 21:01:39.84 +45:56:16.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.331+/-0.035 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4159+45.9379,2461124.9555,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4159+45.9379 20260325.4555 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:39.88 +45:56:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:04.89 +47:19:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.38 21:46:13.65 +43:43:19.4
91.13380 -7.42297 galactic Cyg Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.5487+43.7172 | 21:46:13.65 +43:43:19.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.5487+43.7172,2461124.9555,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.5487+43.7172 20260325.4555 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:13.65 +43:43:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.33 21:02:04.87 +46:52:03.5
87.79115 0.25182 galactic Cyg Second-epoch detections are separated by 1.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5268+46.8598 | 21:02:04.87 +46:52:03.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.553+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5268+46.8598,2461124.9555,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5268+46.8598 20260325.4555 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:04.87 +46:52:03.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.37 21:03:53.32 +43:09:58.8
85.23561 -2.44528 galactic Cyg Second-epoch detections are separated by 2.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:53.32 +43:09:58.8 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:53.32 +43:09:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:23.45 +43:35:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.27 21:02:19.73 +42:51:14.0
84.81226 -2.43950 galactic Cyg Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5775+42.8538 | 21:02:19.73 +42:51:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.487+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5775+42.8538,2461124.9555,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5775+42.8538 20260325.4555 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:19.73 +42:51:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972938586577469952,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972938586577469952 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:38.34 +43:18:23.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.80 21:00:49.09 +46:58:36.9
87.73068 0.48590 galactic Cyg Second-epoch detections are separated by 3.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2176+46.9921 | 21:00:50.84 +46:59:20.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.403+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2176+46.9921,2461124.9555,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2176+46.9921 20260325.4555 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:49.09 +46:58:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:43.22 +46:17:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.18 21:00:54.20 +47:54:28.5
88.44025 1.08887 galactic Cyg Second-epoch detections are separated by 0.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2379+47.9044 | 21:00:54.18 +47:54:29.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.320+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2379+47.9044,2461124.9555,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2379+47.9044 20260325.4555 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:54.20 +47:54:28.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.27 21:00:48.99 +46:02:47.9
87.03100 -0.12719 galactic Cyg Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1990+46.0496 | 21:00:48.99 +46:02:47.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.269+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1990+46.0496,2461124.9555,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1990+46.0496 20260325.4555 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:48.99 +46:02:47.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210051.34+471618.1,2461124.9555,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210051.34+471618.1 20260325.4555 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:51.09 +47:16:30.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.36 21:43:59.41 +43:25:19.2
90.62667 -7.38633 galactic Cyg Second-epoch detections are separated by 2.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972916184027038464 | 21:43:58.05 +43:24:41.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.204+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972916184027038464,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972916184027038464 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:59.41 +43:25:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J211016.72+481849.7,2461124.9555,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J211016.72+481849.7 20260325.4555 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:14.90 +48:18:57.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.16 21:01:45.74 +46:54:02.4
87.77985 0.31452 galactic Cyg Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4396+46.8992 | 21:01:45.74 +46:54:02.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4396+46.8992,2461124.9555,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4396+46.8992 20260325.4555 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:45.74 +46:54:02.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.64 21:02:04.66 +47:33:53.5
88.31320 0.71399 galactic Cyg Second-epoch detections are separated by 2.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5252+47.5700 | 21:02:04.66 +47:33:53.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5252+47.5700,2461124.9555,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5252+47.5700 20260325.4555 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:04.66 +47:33:53.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.49 21:01:17.95 +46:45:47.3
87.62428 0.28307 galactic Cyg Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3320+46.7816 | 21:01:18.66 +46:46:32.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.292+/-0.041 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3320+46.7816,2461124.9555,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3320+46.7816 20260325.4555 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:17.95 +46:45:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:02:46.16 +47:42:36.8
88.49929 0.72315 galactic Cyg Second-epoch detections are separated by 1.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:46.16 +47:42:36.8 (user input) | T | P | (position from user input) J-Ks=0.320+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:46.16 +47:42:36.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5925047,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5925047 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:16.74 +42:26:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165415896685391488,2461124.9555,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165415896685391488 20260325.4555 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:33.87 +47:53:01.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.92 21:02:57.53 +47:28:31.1
88.34485 0.54326 galactic Cyg Second-epoch detections are separated by 0.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7388+47.4728 | 21:02:57.53 +47:28:31.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7388+47.4728,2461124.9555,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7388+47.4728 20260325.4555 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:57.53 +47:28:31.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.35 21:00:43.49 +47:43:24.8
88.28182 0.98989 galactic Cyg Second-epoch detections are separated by 1.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:43.49 +47:43:24.8 (user input) | T | P | (position from user input) J-Ks=1.186+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:43.49 +47:43:24.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165201595011806208,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165201595011806208 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:46.68 +47:28:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.51 21:02:56.66 +46:45:03.2
87.80174 0.06385 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7380+46.7532 | 21:02:56.66 +46:45:03.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.916+/-0.036 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7380+46.7532,2461124.9555,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7380+46.7532 20260325.4555 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:56.66 +46:45:03.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.20 21:46:20.28 +44:04:46.1
91.38277 -7.16383 galactic Cyg Second-epoch detections are separated by 3.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.5877+44.0833 | 21:46:20.25 +44:04:47.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.008+/-0.032 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.5877+44.0833,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.5877+44.0833 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:20.28 +44:04:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163631762967105536,2461124.9555,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163631762967105536 20260325.4555 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:03.42 +46:24:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.43 21:10:33.02 +48:40:56.5
90.09101 0.41855 galactic Cyg Second-epoch detections are separated by 0.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.6375+48.6821 | 21:10:33.02 +48:40:56.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.284+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J317.6375+48.6821,2461124.9555,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.6375+48.6821 20260325.4555 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:33.02 +48:40:56.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.19 21:01:58.90 +47:51:02.7
88.51679 0.91537 galactic Cyg Second-epoch detections are separated by 0.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4814+47.8422 | 21:01:58.91 +47:51:03.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4814+47.8422,2461124.9555,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4814+47.8422 20260325.4555 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:58.90 +47:51:02.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.34 21:40:58.96 +42:53:16.0
89.85565 -7.42678 galactic Cyg Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2460+42.8880 | 21:40:59.05 +42:53:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.354+/-0.030 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2460+42.8880,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2460+42.8880 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:58.96 +42:53:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.14 21:00:51.77 +46:57:05.1
87.71653 0.46335 galactic Cyg Second-epoch detections are separated by 0.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163851252974671104 | 21:00:51.63 +46:57:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.008+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163851252974671104,2461124.9555,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163851252974671104 20260325.4555 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:51.77 +46:57:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.62 21:01:24.12 +47:53:37.8
88.48483 1.01678 galactic Cyg Second-epoch detections are separated by 2.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3461+47.8940 | 21:01:24.12 +47:53:37.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.602+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3461+47.8940,2461124.9555,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3461+47.8940 20260325.4555 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:24.12 +47:53:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.53 21:00:24.83 +47:45:31.2
88.27381 1.05236 galactic Cyg Second-epoch detections are separated by 1.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0850+47.7652 | 21:00:20.50 +47:45:35.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.402+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0850+47.7652,2461124.9555,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0850+47.7652 20260325.4555 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:24.83 +47:45:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.20 21:00:15.24 +47:16:52.5
87.89651 0.75853 galactic Cyg Second-epoch detections are separated by 0.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0638+47.2697 | 21:00:15.24 +47:16:52.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.030+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0638+47.2697,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0638+47.2697 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:15.24 +47:16:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.29 21:01:01.04 +47:07:14.8
87.86120 0.55527 galactic Cyg Second-epoch detections are separated by 1.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:01.04 +47:07:14.8 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:01.04 +47:07:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.28 21:03:11.47 +47:45:34.0
88.58320 0.70283 galactic Cyg Second-epoch detections are separated by 0.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:11.47 +47:45:34.0 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:11.47 +47:45:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210120.64+453647.2,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210120.64+453647.2 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:21.88 +45:36:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.34 21:41:16.45 +42:46:22.6
89.81927 -7.54819 galactic Cyg Second-epoch detections are separated by 0.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3274+42.7757 | 21:41:16.45 +42:46:22.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.310+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.3274+42.7757,2461124.9555,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3274+42.7757 20260325.4555 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:16.45 +42:46:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5840473,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5840473 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:13.39 +47:06:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.45 21:00:57.59 +46:25:05.4
87.32664 0.09918 galactic Cyg Second-epoch detections are separated by 2.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2461+46.4184 | 21:00:57.59 +46:25:05.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.768+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2461+46.4184,2461124.9555,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2461+46.4184 20260325.4555 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:57.59 +46:25:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.36 21:02:45.85 +44:01:19.2
85.73992 -1.72443 galactic Cyg Second-epoch detections are separated by 2.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6903+44.0247 | 21:02:45.85 +44:01:19.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.825+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6903+44.0247,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6903+44.0247 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:45.85 +44:01:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.60 21:02:29.02 +46:43:18.5
87.72760 0.10358 galactic Cyg Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6230+46.7250 | 21:02:29.02 +46:43:18.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.251+/-0.042 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6230+46.7250,2461124.9555,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6230+46.7250 20260325.4555 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:29.02 +46:43:18.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.49 21:01:42.63 +47:57:46.5
88.57084 1.02366 galactic Cyg Second-epoch detections are separated by 0.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4309+47.9613 | 21:01:42.43 +47:57:47.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.376+/-0.026 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4309+47.9613,2461124.9555,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4309+47.9613 20260325.4555 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:42.63 +47:57:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.24 21:02:17.05 +45:55:58.5
87.11417 -0.39365 galactic Cyg Second-epoch detections are separated by 0.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5802+45.9241 | 21:02:17.05 +45:55:58.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.356+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5802+45.9241,2461124.9555,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5802+45.9241 20260325.4555 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:17.05 +45:55:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.01 21:01:17.73 +46:40:29.7
87.55762 0.22528 galactic Cyg Second-epoch detections are separated by 0.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3303+46.6844 | 21:01:17.73 +46:40:29.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.304+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3303+46.6844,2461124.9555,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3303+46.6844 20260325.4555 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:17.73 +46:40:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.77 21:00:00.92 +47:54:55.5
88.34792 1.20583 galactic Cyg Second-epoch detections are separated by 1.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9986+47.9173 | 21:00:00.92 +47:54:55.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.520+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9986+47.9173,2461124.9555,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9986+47.9173 20260325.4555 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:00.92 +47:54:55.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.40 21:01:29.17 +46:29:55.8
87.44707 0.08436 galactic Cyg Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3681+46.4975 | 21:01:29.17 +46:29:55.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.453+/- (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3681+46.4975,2461124.9555,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3681+46.4975 20260325.4555 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:29.17 +46:29:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:04:43.18 +47:51:03.8
88.82260 0.57261 galactic Cyg Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.1760+47.8390 | 21:04:42.24 +47:50:20.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.1760+47.8390,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.1760+47.8390 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:43.18 +47:51:03.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.80 21:00:55.88 +46:42:56.8
87.54711 0.29916 galactic Cyg Second-epoch detections are separated by 0.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2323+46.7160 | 21:00:55.76 +46:42:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.430+/-0.033 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2323+46.7160,2461124.9555,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2323+46.7160 20260325.4555 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:55.88 +46:42:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210152.34+461419.0,2461124.9555,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210152.34+461419.0 20260325.4555 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:50.57 +46:14:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.56 21:01:18.32 +46:38:44.2
87.53673 0.20466 galactic Cyg Second-epoch detections are separated by 4.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3280+46.6499 | 21:01:18.32 +46:38:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3280+46.6499,2461124.9555,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3280+46.6499 20260325.4555 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:18.32 +46:38:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.28 21:01:12.75 +45:54:49.6
86.97654 -0.26654 galactic Cyg Second-epoch detections are separated by 1.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:12.75 +45:54:49.6 (user input) | T | P | (position from user input) J-Ks=0.255+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:12.75 +45:54:49.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.60 21:02:10.79 +47:26:29.8
88.23228 0.61943 galactic Cyg Second-epoch detections are separated by 1.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:10.79 +47:26:29.8 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:10.79 +47:26:29.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.20 21:02:34.91 +46:47:04.7
87.78577 0.13268 galactic Cyg Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6407+46.7855 | 21:02:34.91 +46:47:04.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.824+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6407+46.7855,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6407+46.7855 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:34.91 +46:47:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214634.40+441036.1,2461124.9555,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214634.40+441036.1 20260325.4555 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:34.48 +44:10:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0669 Cyg,2461124.9555,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0669 Cyg 20260325.4555 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:59.36 +45:03:44.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.22 21:01:10.79 +46:46:08.5
87.61521 0.30230 galactic Cyg Second-epoch detections are separated by 1.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:10.79 +46:46:08.5 (user input) | T | P | (position from user input) J-Ks=0.293+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:10.79 +46:46:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163974230786503680,2461124.9555,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163974230786503680 20260325.4555 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:10.42 +47:56:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210107.33+463314.4,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210107.33+463314.4 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:07.13 +46:33:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.52 21:01:00.05 +47:41:38.6
88.29025 0.93553 galactic Cyg Second-epoch detections are separated by 2.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2335+47.6983 | 21:01:00.05 +47:41:38.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.371+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2335+47.6983,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2335+47.6983 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:00.05 +47:41:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.41 21:44:54.86 +43:34:13.9
90.85247 -7.38347 galactic Cyg Second-epoch detections are separated by 0.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.2250+43.5744 | 21:44:54.86 +43:34:13.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.2250+43.5744,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2250+43.5744 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:54.86 +43:34:13.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163971894324282496,2461124.9555,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163971894324282496 20260325.4555 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:14.05 +47:53:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214048.49+421107.7,2461124.9555,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214048.49+421107.7 20260325.4555 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:48.36 +42:11:06.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.95 21:00:45.63 +46:17:54.1
87.21389 0.04604 galactic Cyg Second-epoch detections are separated by 0.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1898+46.2986 | 21:00:45.57 +46:17:55.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.183+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1898+46.2986,2461124.9555,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1898+46.2986 20260325.4555 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:45.63 +46:17:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.35 21:01:02.34 +45:40:24.0
86.77594 -0.40251 galactic Cyg Second-epoch detections are separated by 3.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2479+45.6833 | 21:01:02.34 +45:40:24.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.805+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2479+45.6833,2461124.9555,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2479+45.6833 20260325.4555 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:02.34 +45:40:24.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.82 21:00:20.31 +47:31:07.4
88.08477 0.90401 galactic Cyg Second-epoch detections are separated by 1.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0845+47.5189 | 21:00:20.31 +47:31:07.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.237+/-0.035 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0845+47.5189,2461124.9555,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0845+47.5189 20260325.4555 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:20.31 +47:31:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.19 21:01:04.52 +45:39:42.1
86.77138 -0.41496 galactic Cyg Second-epoch detections are separated by 1.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:04.52 +45:39:42.1 (user input) | T | P | (position from user input) J-Ks=0.264+/-0.032 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:04.52 +45:39:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.47 21:01:32.66 +47:50:45.8
88.46473 0.96730 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:32.66 +47:50:45.8 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:32.66 +47:50:45.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.23 21:00:12.39 +47:32:58.4
88.09334 0.94107 galactic Cyg Second-epoch detections are separated by 0.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0355+47.5426 | 21:00:12.39 +47:32:58.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.120+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0355+47.5426,2461124.9555,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0355+47.5426 20260325.4555 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:12.39 +47:32:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.86 21:41:28.34 +42:57:28.9
89.97030 -7.43351 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1966923124102435200 | 21:41:28.34 +42:57:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.157+/-0.027 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966923124102435200,2461124.9555,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966923124102435200 20260325.4555 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:28.34 +42:57:28.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:09.12 +42:18:06.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.12 21:00:20.56 +47:32:40.1
88.10463 0.92042 galactic Cyg Second-epoch detections are separated by 1.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:20.56 +47:32:40.1 (user input) | T | P | (position from user input) J-Ks=0.585+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:20.56 +47:32:40.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.32 21:01:13.23 +46:58:38.3
87.77625 0.43458 galactic Cyg Second-epoch detections are separated by 1.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2832+46.9721 | 21:01:12.41 +46:58:08.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.006+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2832+46.9721,2461124.9555,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2832+46.9721 20260325.4555 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:13.23 +46:58:38.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.21 21:42:07.74 +43:21:56.0
90.33236 -7.20667 galactic Cyg Second-epoch detections are separated by 1.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5204+43.3581 | 21:42:07.74 +43:21:56.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.986+/-0.029 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5204+43.3581,2461124.9555,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5204+43.3581 20260325.4555 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:07.74 +43:21:56.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.15 21:43:01.85 +43:44:28.6
90.70556 -7.03138 galactic Cyg Second-epoch detections are separated by 1.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.7537+43.7435 | 21:43:01.85 +43:44:28.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.348+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.7537+43.7435,2461124.9555,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7537+43.7435 20260325.4555 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:01.85 +43:44:28.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.70 21:01:09.91 +47:44:33.2
88.34494 0.94676 galactic Cyg Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2922+47.7416 | 21:01:09.91 +47:44:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.431+/-0.082 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2922+47.7416,2461124.9555,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2922+47.7416 20260325.4555 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:09.91 +47:44:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.82 21:00:51.08 +46:38:28.1
87.48195 0.26025 galactic Cyg Second-epoch detections are separated by 0.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163652413169801728 | 21:00:50.99 +46:38:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.278+/-0.036 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163652413169801728,2461124.9555,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163652413169801728 20260325.4555 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:51.08 +46:38:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.83 22:10:52.94 +49:38:37.7
98.14460 -5.34184 galactic Lac Second-epoch detections are separated by 2.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976712625885317504 | 22:10:52.95 +49:38:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.715+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976712625885317504,2461124.9555,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976712625885317504 20260325.4555 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:10:52.94 +49:38:37.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.52 21:00:58.52 +46:58:58.6
87.75289 0.46972 galactic Cyg Second-epoch detections are separated by 0.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:58.52 +46:58:58.6 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:58.52 +46:58:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.44 21:00:16.81 +47:41:00.9
88.20247 1.01988 galactic Cyg Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0638+47.6720 | 21:00:16.84 +47:41:01.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.502+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0638+47.6720,2461124.9555,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0638+47.6720 20260325.4555 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:16.81 +47:41:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.89 21:01:46.38 +43:42:50.7
85.39074 -1.79453 galactic Cyg Second-epoch detections are separated by 2.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:46.38 +43:42:50.7 (user input) | T | P | (position from user input) J-Ks=0.449+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:46.38 +43:42:50.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.65 21:04:18.36 +47:48:57.0
88.75001 0.60074 galactic Cyg Second-epoch detections are separated by 6.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.0814+47.8217 | 21:04:18.36 +47:48:57.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.0814+47.8217,2461124.9555,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.0814+47.8217 20260325.4555 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:18.36 +47:48:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.63 21:03:25.10 +46:44:04.1
87.84347 -0.00772 galactic Cyg Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.8648+46.7428 | 21:03:25.10 +46:44:04.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.135+/-0.032 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.8648+46.7428,2461124.9555,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.8648+46.7428 20260325.4555 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:25.10 +46:44:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.16 21:02:57.56 +47:27:45.7
88.33548 0.53481 galactic Cyg Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7388+47.4728 | 21:02:57.56 +47:27:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.458+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7388+47.4728,2461124.9555,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7388+47.4728 20260325.4555 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:57.56 +47:27:45.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.20 21:00:52.11 +46:49:27.3
87.62156 0.37878 galactic Cyg Second-epoch detections are separated by 1.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:52.11 +46:49:27.3 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:52.11 +46:49:27.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210045.47+473008.1,2461124.9555,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210045.47+473008.1 20260325.4555 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:45.51 +47:30:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163957463234337792,2461124.9555,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163957463234337792 20260325.4555 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:04.72 +47:48:55.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.39 21:01:23.37 +47:05:14.4
87.87789 0.48562 galactic Cyg Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:23.37 +47:05:14.4 (user input) | T | P | (position from user input) J-Ks=0.631+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:23.37 +47:05:14.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.47 21:02:36.73 +47:02:34.5
87.98245 0.30017 galactic Cyg Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:36.73 +47:02:34.5 (user input) | T | P | (position from user input) J-Ks=0.800+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:36.73 +47:02:34.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.79 21:02:38.80 +47:33:01.7
88.36607 0.63258 galactic Cyg Second-epoch detections are separated by 2.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2165392703846730112 | 21:02:39.03 +47:33:28.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2165392703846730112,2461124.9555,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2165392703846730112 20260325.4555 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:38.80 +47:33:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.09 21:00:06.21 +47:39:07.4
88.15915 1.02155 galactic Cyg Second-epoch detections are separated by 0.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0342+47.6405 | 21:00:06.21 +47:39:07.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.287+/-0.037 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0342+47.6405,2461124.9555,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0342+47.6405 20260325.4555 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:06.21 +47:39:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.50 21:42:18.50 +43:17:39.2
90.30967 -7.28180 galactic Cyg Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:18.50 +43:17:39.2 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=1.009+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:18.50 +43:17:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.56 21:48:27.62 +44:51:17.4
92.17820 -6.81565 galactic Cyg Second-epoch detections are separated by 1.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.1168+44.8568 | 21:48:27.62 +44:51:17.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.756+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.1168+44.8568,2461124.9555,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1168+44.8568 20260325.4555 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:27.62 +44:51:17.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1969596552264122752,2461124.9555,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1969596552264122752 20260325.4555 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:39.39 +42:08:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.68 21:01:23.78 +47:15:38.4
88.00879 0.59925 galactic Cyg Second-epoch detections are separated by 1.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:23.78 +47:15:38.4 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:23.78 +47:15:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.12 21:00:20.53 +47:35:01.6
88.13417 0.94635 galactic Cyg Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0912+47.5838 | 21:00:20.47 +47:35:02.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.808+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0912+47.5838,2461124.9555,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0912+47.5838 20260325.4555 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:20.53 +47:35:01.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163650390246885376,2461124.9555,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163650390246885376 20260325.4555 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:30.78 +46:33:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.46 21:45:19.54 +43:43:55.8
91.01559 -7.30938 galactic Cyg Second-epoch detections are separated by 0.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.3233+43.7386 | 21:45:19.54 +43:43:55.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.828+/-0.029 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.3233+43.7386,2461124.9555,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.3233+43.7386 20260325.4555 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:19.54 +43:43:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:45.20 +47:29:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163955809653800960,2461124.9555,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163955809653800960 20260325.4555 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:07.55 +47:42:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.32 21:46:50.91 +43:45:47.6
91.24685 -7.46431 galactic Cyg Second-epoch detections are separated by 0.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1973007237334027520 | 21:46:51.85 +43:45:03.4 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE J-Ks=0.681+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973007237334027520,2461124.9555,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973007237334027520 20260325.4555 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:50.91 +43:45:47.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.41 21:01:42.57 +42:56:49.8
84.80720 -2.29273 galactic Cyg Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4315+42.9483 | 21:01:42.57 +42:56:49.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.145+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4315+42.9483,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4315+42.9483 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:42.57 +42:56:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163531952233476608,2461124.9555,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163531952233476608 20260325.4555 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:53.18 +46:05:45.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.66 21:00:33.77 +47:46:33.7
88.30337 1.04494 galactic Cyg Second-epoch detections are separated by 0.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1427+47.7797 | 21:00:33.77 +47:46:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.372+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1427+47.7797,2461124.9555,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1427+47.7797 20260325.4555 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:33.77 +47:46:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.80 21:02:22.01 +47:34:49.1
88.35709 0.68769 galactic Cyg Second-epoch detections are separated by 1.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2165404661050390912 | 21:02:21.92 +47:34:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.247+/-0.056 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165404661050390912,2461124.9555,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165404661050390912 20260325.4555 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:22.01 +47:34:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.62 22:09:29.70 +49:22:38.6
97.80530 -5.42894 galactic Lac Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1976684863216153216 | 22:09:30.25 +49:22:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1976684863216153216,2461124.9555,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1976684863216153216 20260325.4555 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:29.70 +49:22:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.75 21:02:07.48 +43:22:28.0
85.17805 -2.06698 galactic Cyg Second-epoch detections are separated by 1.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5307+43.3748 | 21:02:07.48 +43:22:28.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.535+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5307+43.3748,2461124.9555,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.5307+43.3748 20260325.4555 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:07.48 +43:22:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.45 21:00:40.04 +47:48:49.8
88.34338 1.05664 galactic Cyg Second-epoch detections are separated by 1.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:40.04 +47:48:49.8 (user input) | T | P | (position from user input) J-Ks=1.139+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:40.04 +47:48:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.39 21:00:58.41 +47:25:47.5
88.08861 0.76474 galactic Cyg Second-epoch detections are separated by 0.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2430+47.4305 | 21:00:58.33 +47:25:49.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2430+47.4305,2461124.9555,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2430+47.4305 20260325.4555 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:58.41 +47:25:47.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
PMAK V20,2461124.9555,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PMAK V20 20260325.4555 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:41.77 +43:56:20.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.20 21:01:03.89 +47:20:01.0
88.02647 0.68962 galactic Cyg Second-epoch detections are separated by 1.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2617+47.3407 | 21:01:03.89 +47:20:01.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2617+47.3407,2461124.9555,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2617+47.3407 20260325.4555 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:03.89 +47:20:01.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.33 21:00:34.61 +46:56:48.7
87.68093 0.49706 galactic Cyg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163852730445202304 | 21:00:35.87 +46:57:26.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.376+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163852730445202304,2461124.9555,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163852730445202304 20260325.4555 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:34.61 +46:56:48.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.27 21:41:42.49 +42:28:26.3
89.67995 -7.82513 galactic Cyg Second-epoch detections are separated by 2.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:42.49 +42:28:26.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.867+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:42.49 +42:28:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J220651.58+490707.1,2461124.9555,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220651.58+490707.1 20260325.4555 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:51.26 +49:07:03.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.18 21:41:42.58 +43:28:15.8
90.34489 -7.07715 galactic Cyg Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4269+43.4715 | 21:41:42.47 +43:28:17.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5) J-Ks=1.278+/-0.029 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4269+43.4715,2461124.9555,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4269+43.4715 20260325.4555 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:42.58 +43:28:15.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.10 21:42:55.45 +43:13:24.3
90.34774 -7.40892 galactic Cyg Second-epoch detections are separated by 1.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:55.45 +43:13:24.3 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=1.043+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:55.45 +43:13:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.54 21:01:20.96 +47:10:44.2
87.94216 0.55126 galactic Cyg Second-epoch detections are separated by 0.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3386+47.1904 | 21:01:20.96 +47:10:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3386+47.1904,2461124.9555,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3386+47.1904 20260325.4555 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:20.96 +47:10:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163590295076582016,2461124.9555,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163590295076582016 20260325.4555 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:45.62 +46:26:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165403836417235840,2461124.9555,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165403836417235840 20260325.4555 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:40.21 +47:51:05.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.38 21:46:00.54 +44:26:43.7
91.57671 -6.84701 galactic Cyg Second-epoch detections are separated by 1.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.4991+44.4415 | 21:46:00.54 +44:26:43.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.333+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.4991+44.4415,2461124.9555,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.4991+44.4415 20260325.4555 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:00.54 +44:26:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.39 21:03:44.95 +47:40:16.8
88.57990 0.57414 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.9372+47.6663 | 21:03:44.95 +47:40:16.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.512+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.9372+47.6663,2461124.9555,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.9372+47.6663 20260325.4555 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:44.95 +47:40:16.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.18 21:01:59.98 +47:07:19.4
87.97260 0.43070 galactic Cyg Second-epoch detections are separated by 0.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4926+47.1234 | 21:01:59.98 +47:07:19.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.319+/-0.030 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4926+47.1234,2461124.9555,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4926+47.1234 20260325.4555 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:59.98 +47:07:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:17.91 +47:39:14.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.43 21:01:36.54 +47:07:10.9
87.92686 0.47897 galactic Cyg Second-epoch detections are separated by 2.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3894+47.1256 | 21:01:36.54 +47:07:10.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.116+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3894+47.1256,2461124.9555,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3894+47.1256 20260325.4555 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:36.54 +47:07:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165395276533453824,2461124.9555,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165395276533453824 20260325.4555 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:14.96 +47:40:60.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163905335200296320,2461124.9555,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163905335200296320 20260325.4555 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:10.40 +47:31:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.23 21:01:16.29 +47:39:54.8
88.29866 0.88227 galactic Cyg Second-epoch detections are separated by 1.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:16.29 +47:39:54.8 (user input) | T | P | (position from user input) J-Ks=1.266+/-0.045 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:16.29 +47:39:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.66 21:01:05.42 +46:49:26.4
87.64640 0.35009 galactic Cyg Second-epoch detections are separated by 1.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2740+46.8245 | 21:01:05.42 +46:49:26.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2740+46.8245,2461124.9555,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2740+46.8245 20260325.4555 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:05.42 +46:49:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J210148.9+472744,2461124.9555,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J210148.9+472744 20260325.4555 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:48.86 +47:27:56.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163636268409059072,2461124.9555,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163636268409059072 20260325.4555 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:40.49 +46:31:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.96 21:42:35.88 +43:06:07.4
90.22202 -7.46113 galactic Cyg Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972883194377238144 | 21:42:35.86 +43:06:08.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.197+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972883194377238144,2461124.9555,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972883194377238144 20260325.4555 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:35.88 +43:06:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210144.04+460541.8,2461124.9555,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210144.04+460541.8 20260325.4555 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:42.60 +46:05:33.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:10.62 +43:40:56.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.26 21:01:17.70 +46:39:32.3
87.54559 0.21481 galactic Cyg Second-epoch detections are separated by 0.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3280+46.6499 | 21:01:17.70 +46:39:32.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.999+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3280+46.6499,2461124.9555,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3280+46.6499 20260325.4555 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:17.70 +46:39:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.18 21:02:46.06 +47:00:34.9
87.97519 0.25830 galactic Cyg Second-epoch detections are separated by 0.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6915+47.0189 | 21:02:46.06 +47:00:34.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.717+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.6915+47.0189,2461124.9555,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6915+47.0189 20260325.4555 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:46.06 +47:00:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.97 21:01:19.42 +46:58:50.7
87.79045 0.42364 galactic Cyg Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3199+46.9908 | 21:01:19.26 +46:58:52.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.082+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3199+46.9908,2461124.9555,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3199+46.9908 20260325.4555 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:19.42 +46:58:50.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973611865649234560,2461124.9555,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973611865649234560 20260325.4555 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:55.68 +45:48:32.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:26.30 +47:45:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163973887189213696,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163973887189213696 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:29.52 +47:56:56.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213538.63+453419.7,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213538.63+453419.7 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:38.64 +45:34:17.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.69 21:00:48.99 +46:29:42.1
87.36814 0.16842 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2041+46.4952 | 21:00:48.99 +46:29:43.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.683+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2041+46.4952,2461124.9555,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2041+46.4952 20260325.4555 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:48.99 +46:29:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.07 21:01:11.38 +47:47:18.4
88.38214 0.97396 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163957188356437888 | 21:01:11.50 +47:47:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163957188356437888,2461124.9555,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163957188356437888 20260325.4555 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:11.38 +47:47:18.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.04 21:03:08.72 +47:36:12.4
88.46153 0.60489 galactic Cyg Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7870+47.6065 | 21:03:08.72 +47:36:12.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.338+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7870+47.6065,2461124.9555,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7870+47.6065 20260325.4555 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:08.72 +47:36:12.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.37 21:01:08.77 +47:09:53.6
87.90880 0.56791 galactic Cyg Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:08.77 +47:09:53.6 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:08.77 +47:09:53.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.41 21:02:00.34 +44:02:06.9
85.65947 -1.61354 galactic Cyg Second-epoch detections are separated by 0.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:00.34 +44:02:06.9 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:00.34 +44:02:06.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.81 21:00:29.82 +47:52:19.3
88.36836 1.11647 galactic Cyg Second-epoch detections are separated by 1.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:29.82 +47:52:19.3 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:29.82 +47:52:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J221206.95+493238.4,2461124.9555,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221206.95+493238.4 20260325.4555 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:06.72 +49:32:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.29 21:46:41.09 +43:22:37.1
90.97167 -7.73939 galactic Cyg Second-epoch detections are separated by 0.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:41.09 +43:22:37.1 (user input) | T | P | (position from user input) J-Ks=1.110+/-0.036 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:41.09 +43:22:37.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.79 22:09:11.03 +49:35:48.1
97.89191 -5.22106 galactic Lac Second-epoch detections are separated by 1.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.3124+49.5928 | 22:09:11.29 +49:35:51.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.3124+49.5928,2461124.9555,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.3124+49.5928 20260325.4555 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:11.03 +49:35:48.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.68 21:01:14.98 +47:20:40.5
88.05538 0.67334 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163894683680372864 | 21:01:14.88 +47:20:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.293+/-0.039 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163894683680372864,2461124.9555,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163894683680372864 20260325.4555 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:14.98 +47:20:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.01 21:00:39.55 +47:49:42.1
88.35341 1.06724 galactic Cyg Second-epoch detections are separated by 0.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1627+47.8346 | 21:00:39.54 +47:49:42.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.452+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1627+47.8346,2461124.9555,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1627+47.8346 20260325.4555 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:39.55 +47:49:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9555,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4555 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:24.76 +47:29:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.54 21:03:43.86 +47:57:01.8
88.78609 0.76238 galactic Cyg Second-epoch detections are separated by 2.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.9287+47.9528 | 21:03:43.86 +47:57:01.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.772+/-0.027 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.9287+47.9528,2461124.9555,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.9287+47.9528 20260325.4555 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:43.86 +47:57:01.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.30 21:01:32.17 +47:44:22.2
88.38385 0.89791 galactic Cyg Second-epoch detections are separated by 4.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3848+47.7397 | 21:01:32.17 +47:44:22.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.880+/-0.040 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.3848+47.7397,2461124.9555,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.3848+47.7397 20260325.4555 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:32.17 +47:44:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.41 21:02:53.71 +43:52:57.2
85.65121 -1.83461 galactic Cyg Second-epoch detections are separated by 0.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7237+43.8827 | 21:02:53.71 +43:52:57.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.474+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.7237+43.8827,2461124.9555,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.7237+43.8827 20260325.4555 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:53.71 +43:52:57.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 11.87 21:02:30.15 +47:38:53.2
88.42301 0.71554 galactic Cyg Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2165405447015665408 | 21:02:30.08 +47:38:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.984+/-0.037 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2165405447015665408,2461124.9555,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2165405447015665408 20260325.4555 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:30.15 +47:38:53.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.07 21:00:22.20 +46:58:48.4
87.68272 0.54552 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2163853731180833408 | 21:00:22.09 +46:58:49.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.271+/-0.028 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163853731180833408,2461124.9555,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163853731180833408 20260325.4555 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:22.20 +46:58:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4555 2461124.9555 12.44 21:40:57.21 +42:29:09.1
89.58271 -7.72404 galactic Cyg Second-epoch detections are separated by 1.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2366+42.4829 | 21:40:57.21 +42:29:09.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2366+42.4829,2461124.9555,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2366+42.4829 20260325.4555 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:57.21 +42:29:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163974402585178752,2461124.9555,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163974402585178752 20260325.4555 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:06.14 +47:56:10.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2163646778172750080,2461124.9555,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2163646778172750080 20260325.4555 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:33.85 +46:28:25.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20_00sec_-14_90C_LIGHT_0181_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461124.95572647 25.03.2026 10:56:04.767 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.07
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 26768
Objects passed selection criteria: 26584
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 16453
Average stars matched: 15368 (93.4055 %)
Memory usage VmPeak: 130180 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 05:58:26 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461124.95572647 25.03.2026 10:56:04.767 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 606
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 184 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 199042
Objects passed selection criteria: 198456
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 132131
Average stars matched: 122313 (92.5693 %)
Memory usage VmPeak: 2213044 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 06:05:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461124.95519410
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
Saving wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits to local_wcs_cache/
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
Saving wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits to local_wcs_cache/
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits'
wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:36:09.923 +45:57:58.59
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:36:08.212 +45:57:52.56
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:36:09.923 +45:57:58.59
Second-epoch second image center 21:36:08.212 +45:57:52.56
Angular distance between the image centers 0.00523 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.G64lHmyjgk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.qLSN5W0G6F
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.TNI2nhWpBC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits &> /tmp/tmp.tnRqCdAmpn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 14243 out of 30795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.935356
a=0.000000 b=1.000000 c=22.935356
From vast_summary.log: estimated ref. image limiting mag.: -8.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.87
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.87
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
2.4 pix Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
2.3 pix fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
2.3 pix fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Limiting magnitude estimates:
14.9 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
14.9 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
12.4 mag. fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
12.5 mag. fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.G64lHmyjgk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3934, passed=30795
Got 30795 stars (including 26843 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 30795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qLSN5W0G6F (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3890, passed=30626
Got 30626 stars (including 26706 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 30626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TNI2nhWpBC (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=448, passed=7072
Got 7072 stars (including 6617 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 7072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 944 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tnRqCdAmpn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=412, passed=6303
Got 6303 stars (including 5881 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat
util/solve_plate_with_UCAC5 got 6303 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 950 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits'
Preparing the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out10437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24118.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21306_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 21306_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11121_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 11121_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12172_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 12172_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10538_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 10538_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10437_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 10437_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24118_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 24118_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12359_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 12359_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11831_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 11831_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 17s
Prepared the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:00:36.46 +47:54:44.4
21:01:04.14 +47:53:15.6
21:00:49.41 +47:42:57.7
21:00:33.37 +47:29:25.6
21:00:34.83 +47:23:01.6
21:08:45.05 +47:24:08.6
21:45:29.24 +44:32:48.5
21:41:56.50 +43:29:18.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Creating symlink local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:36:09.923 +45:57:58.59
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:36:08.212 +45:57:52.56
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:36:09.923 +45:57:58.59
Second-epoch second image center 21:36:08.212 +45:57:52.56
Angular distance between the image centers 0.00523 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.4lUgknSqzg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.rFpkR26ODG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.UCrE6TZdsO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits &> /tmp/tmp.9IWKs0V3XP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 15408 out of 227547 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.745984
a=0.000000 b=1.000000 c=22.745984
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 557 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
2.2 pix Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
2.3 pix fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
2.2 pix fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Limiting magnitude estimates:
15.0 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
15.0 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
12.9 mag. fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
12.9 mag. fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4lUgknSqzg (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=44928, passed=227506
Got 227506 stars (including 182305 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 227506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rFpkR26ODG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=45138, passed=228742
Got 228742 stars (including 183314 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 228742 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UCrE6TZdsO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=4256, passed=65132
Got 65132 stars (including 60796 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 65132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 946 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9IWKs0V3XP (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3831, passed=60013
Got 60013 stars (including 56111 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat
util/solve_plate_with_UCAC5 got 60013 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-55-18_20.00sec_-14.90C_LIGHT_0181.fits
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cyg-04-Q2b1x1_055644_TTUQ2b1x1_16558_jOLapFK7/wcs_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182.fits
Preparing the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out240411.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_local.txt__out171889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172422.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out172594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173939.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out174599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174849.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out175284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out181692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out181901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out182307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183011.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out183567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out224729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out225037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257974.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out258007.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out27594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53189.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out73548.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out74833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74842.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out75121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76306.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out76388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76455.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out76597.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out76834.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out76992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77304.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out77385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77946.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out78099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78677.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out79052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79783.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out82420.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out84643.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out87186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87588.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out87903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88328.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out88614.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out93998.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out94649.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out94806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95384.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out95853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96278.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out96828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99803.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 432s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 181s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257947_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257947_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:44:19.25 +43:46:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.399 1972977103845152000 326.08026817448 +43.77199829710 13.1432 12.1684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257950_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257950_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:29:06.08 +43:58:34.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257952_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257952_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:23:23.33 +46:22:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257953_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257953_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:11:24.19 +44:57:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.127 2162478860611053568 317.85125380400 +44.96479782611 13.0633 12.7298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257955_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257955_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:06:48.18 +47:44:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.343 2165224787836628480 316.70082776564 +47.73398035050 13.0427 12.4881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257958_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257958_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:04:21.48 +47:12:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.331 2165182147399310848 316.08939275715 +47.20302899678 13.2970 12.9914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257962_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257962_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:30:23.81 +46:19:46.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)
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Considering the candidate 257969_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257969_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:32:28.67 +44:29:13.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)
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Considering the candidate 257970_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257970_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:27:55.31 +45:13:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.423 1971283718505428352 321.98013014819 +45.22879282372 12.3924 11.5532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257974_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 257974_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 257978_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257978_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:03:00.46 +46:37:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.316 2163663309524170496 315.75106898242 +46.62147613454 13.3481 12.4967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257983_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257983_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:58:30.06 +48:06:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.087 1976185062154385024 329.62499599751 +48.10750017067 12.3123 11.5495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257984_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 257984_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 257985_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257985_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:14:33.80 +44:07:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.473 1970042777882329600 318.64075367162 +44.13129405956 12.2782 11.2783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257986_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257986_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:42:12.45 +42:50:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257988_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257988_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 22:02:37.31 +47:06:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 5.422 1975278656559928832 330.65717845417 +47.10458044349 12.1523 11.7698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257992_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257992_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:29:39.10 +43:39:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 1.150 1970891880047316352 322.41321903072 +43.66392741212 12.1342 11.6574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257996_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257996_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:05:52.56 +42:12:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.584 1969635649343637888 316.46901140350 +42.21008804916 13.0872 12.5168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257997_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 257997_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:55:42.30 +48:22:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.811 1976350474242447744 328.92549322354 +48.37840836190 11.9746 11.5004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258001_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258001_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:16:08.85 +47:29:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 5.074 2164826524092861440 319.03496580418 +47.48912658533 12.0241 11.0110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258003_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258003_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:50:20.73 +46:20:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.528 1974482094744062976 327.58647537921 +46.33632381009 11.3122 10.1642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258004_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258004_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:17:53.15 +48:32:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.747 2164988221018468992 319.47175005226 +48.54039644071 11.7946 11.2357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258007_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 258007_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 258008_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258008_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:40:21.98 +44:15:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 2.993 1973787993671594240 325.09274051777 +44.26523693027 11.8018 11.0369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258009_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258009_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:03:50.82 +42:11:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.711 1969597445622248832 315.96199180853 +42.18455506827 12.6451 11.9790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258010_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258010_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:39:11.25 +48:11:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 0.657 1978018845696435200 324.79689989359 +48.19256833467 11.3345 11.0023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258011_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258011_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:16:22.25 +47:09:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.904 2164255259091693312 319.09270627662 +47.16611216132 11.1585 10.1004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258015_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258015_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:03:31.99 +45:37:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.031 2162708173196326400 315.88293050177 +45.62121841972 12.0937 11.6438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258016_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258016_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:06:04.05 +43:52:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 1.438 2162317747793836032 316.51708117286 +43.88234302528 11.7312 11.2733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258018_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 258018_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:06:20.20 +44:53:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 2.919 2162430035421671040 316.58476401222 +44.89052482697 11.1703 10.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 260823_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 260823_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 260829_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 260829_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:04:03.53 +42:25:20.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)
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Considering the candidate 260852_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 260852_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:10:08.78 +43:59:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.712 1970259626506947712 317.53663379403 +43.99263875576 11.2695 10.8337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 261555_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 261555_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:57:06.69 +48:39:46.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262712_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 262712_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:13:06.65 +46:46:15.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)
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Considering the candidate 262914_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 262914_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:33:11.81 +45:50:00.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263406_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 263406_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:56:25.17 +47:29:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)GAIADR2_OUTPUT=# 1.466 1976041167874761728 329.10535605498 +47.48935636435 11.3068 10.4359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 263431_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 263431_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:02:51.69 +46:29:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.963 2163591978703794048 315.71542897764 +46.49090369727 12.5650 12.2875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 263457_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 263457_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 263486_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 263486_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:10:39.59 +47:41:52.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263945_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 263945_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 264059_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 264059_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:47:50.90 +45:00:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.567 1973890420052564224 326.96234480512 +45.00703306004 11.8444 11.1324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264698_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 264698_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 22:08:59.10 +48:31:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264855_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 264855_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:21:08.10 +41:59:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265139_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 265139_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:34:25.22 +45:59:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.686 1977370576209979520 323.60517675530 +45.99696376875 12.0005 11.6497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265141_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 265141_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:02:01.83 +46:16:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.227 2163582976451468032 315.50851643337 +46.27291671319 12.9124 12.1588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265239_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 265239_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 22:05:53.58 +48:16:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 2.604 1975771237771587712 331.47334946228 +48.26830361345 11.1510 10.0292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265559_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 265559_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:39:20.58 +41:43:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 1.781 1966524448057003776 324.83514494283 +41.72722997480 12.0251 11.6836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265604_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 265604_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:06:10.72 +47:10:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 0.573 2165137101779878016 316.54458849788 +47.17628885346 12.2614 11.2739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265853_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 265853_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:54:41.31 +47:29:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 2.854 1976050754241212032 328.67315833089 +47.49345806597 11.9163 11.1757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 266315_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 266315_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:19:33.36 +49:29:23.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266330_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 266330_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:03:10.76 +41:34:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266409_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 266409_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:41:51.50 +45:45:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266758_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 266758_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:13:42.81 +45:38:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 5.064 2164021814710312704 318.42950617314 +45.64774661470 12.0453 11.7646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267162_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 267162_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:04:15.21 +46:31:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.297 2163612697627752192 316.06292565195 +46.52024062367 12.8348 12.1864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267338_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 267338_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:05:01.68 +46:31:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.145 2163606203636746112 316.25670035161 +46.53282562316 12.5462 11.6960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267349_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 267349_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:29:22.73 +46:30:34.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 267431_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 267431_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:06:00.87 +46:16:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.958 2162846230621767680 316.50365811957 +46.28304300549 12.1854 11.4397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267467_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 267467_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:10:38.97 +47:40:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 267738_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 267738_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 22:08:19.32 +49:14:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 2.673 1976677334126685568 332.08119527056 +49.23814327532 11.7685 10.9648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268175_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 268175_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:07:20.57 +46:10:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.495 2162830425142152576 316.83590287995 +46.17113906501 12.1270 11.0454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268536_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 268536_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:07:21.13 +44:40:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.324 2162503118588036608 316.83894131797 +44.67396924399 13.0435 12.5209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268673_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 268673_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 269129_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269129_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:12:07.60 +45:29:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.836 2164007658498152832 318.03140363701 +45.48911342034 12.7118 12.4208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269167_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269167_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:55:12.77 +47:26:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.513 1976052231710004864 328.80340100294 +47.43416428233 12.4226 11.9414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269201_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269201_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:59:42.18 +49:05:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.528 1976484923896170752 329.92595686148 +49.09799902109 11.7176 11.5633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269272_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269272_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:31:30.31 +47:16:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 1.115 1978240775252407680 322.87630825442 +47.27122630346 11.6553 10.8474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269366_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269366_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:37:59.61 +48:28:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.768 1978788606919678208 324.49862691899 +48.47243846270 11.1572 10.0398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269446_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269446_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:24:52.24 +46:30:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269531_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269531_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:05:40.87 +46:40:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.433 2163608746257698176 316.42121146189 +46.66801912551 12.8622 12.0150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269552_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269552_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:06:38.60 +47:15:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.310 2165139232083921152 316.66176175255 +47.26023913276 13.2363 12.8716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 269940_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269940_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:03:37.79 +45:23:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269944_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 269944_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:43:39.18 +44:32:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 3.477 1973862485583620736 325.91435052855 +44.53720225129 12.5624 11.7781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 270196_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 270196_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:07:34.56 +42:56:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.596 1970065459620881024 316.89423399587 +42.94353371602 12.9525 12.3068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 270283_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 270283_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:44:41.96 +43:45:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270332_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 270332_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:09:00.42 +45:16:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.913 2162544144116244352 317.25177880818 +45.27422551443 13.0253 12.4911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 270557_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 270557_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:10:06.93 +45:30:39.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 270591_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 270591_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:06:10.98 +43:48:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.093 2162305236541117440 316.54521423104 +43.80690651356 13.3135 12.5934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 270610_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 270610_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:35:50.17 +45:24:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270840_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 270840_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:31:53.58 +41:44:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.896 1967143129506289408 322.97341402619 +41.74563325409 12.5882 11.9993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271327_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 271327_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:51:21.44 +44:39:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271366_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 271366_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:41:48.19 +45:45:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271531_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 271531_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:15:10.69 +42:57:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.382 1969913276031960192 318.79408443060 +42.95822826313 12.5889 11.6942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271539_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 271539_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:53:25.69 +42:43:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 5.076 1960666009585015040 328.35860355483 +42.73056987368 12.6474 11.8039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 271628_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 271628_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:29:17.89 +46:31:33.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 271943_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 271943_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:32:20.11 +48:38:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272070_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 272070_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:28:44.50 +49:48:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.931 2170973236462665600 322.18503675950 +49.80525481291 11.5098 11.2282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 272353_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 272353_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 272433_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 272433_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:38:49.17 +41:42:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 3.911 1966710501739223168 324.70531016828 +41.71042559725 12.6279 11.5809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 272882_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 272882_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:35:39.02 +42:51:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.124 1967577951995108096 323.91212928775 +42.86509815773 12.9584 12.3685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 272883_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 272883_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:41:13.36 +47:33:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.804 1977931262721180672 325.30546865625 +47.56617742220 11.0848 9.7679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 273334_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 273334_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:17:20.57 +48:01:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.011 2164867206023855232 319.33538606356 +48.03056883818 12.8137 12.3571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 273389_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 273389_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:40:23.52 +43:15:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 273427_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 273427_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:33:42.73 +44:34:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.194 1971039901799006720 323.42774499481 +44.56775052846 12.5680 11.7749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 273644_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 273644_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:46:26.01 +44:17:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.636 1973085852416990464 326.60745856469 +44.28582332784 13.1090 12.3706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 273688_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 273688_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 273922_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 273922_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:29:42.62 +46:56:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 0.673 1972224728664504448 322.42760811902 +46.94401938073 11.1599 9.7589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 274118_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 274118_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 274348_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 274348_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 274690_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 274690_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:51:50.26 +46:11:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.640 1974427355376033536 327.95880887798 +46.18631316783 12.4156 11.4111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 274840_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 274840_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:29:31.19 +46:56:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.089 1972271526630987392 322.37994074942 +46.93429952996 12.5837 11.8068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 275071_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 275071_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 275090_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 275090_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 275138_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 275138_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:56:59.12 +45:47:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.378 1973611036716313216 329.24551897872 +45.79428182970 12.9082 12.6854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105506_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 105506_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 240411_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 240411_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:38:46.60 +43:39:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.318 1967765350009518208 324.69409836034 +43.65601013639 13.0356 12.3058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182307_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 182307_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 119721_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 119721_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 74833_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74833_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 53189_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 53189_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 115904_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 115904_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 222361_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 222361_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 172228_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 172228_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85201_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85201_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 106851_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 106851_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 174599_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 174599_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 181901_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 181901_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 116562_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 116562_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 193723_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 193723_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 199828_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 199828_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 118609_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 118609_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89774_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89774_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 36853_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 36853_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 166051_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 166051_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91910_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91910_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 110801_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 110801_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97759_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97759_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 25620_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 25620_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89591_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89591_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87803_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87803_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 130655_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 130655_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:38:31.86 +45:42:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87983_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87983_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 95876_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 95876_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 194235_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 194235_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 93836_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93836_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 74867_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74867_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97025_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97025_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 168920_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 168920_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 114177_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 114177_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 166052_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 166052_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87882_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87882_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 84643_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 84643_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 194171_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 194171_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 169481_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 169481_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 191053_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 191053_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 190664_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 190664_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 116446_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 116446_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 41779_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 41779_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 162807_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 162807_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 196532_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 196532_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 157103_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 157103_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78248_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78248_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 100669_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 100669_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 171594_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 171594_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78098_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78098_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76388_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76388_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 105895_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 105895_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 168368_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 168368_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 171646_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 171646_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 93982_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93982_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83944_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83944_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 80546_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80546_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82453_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82453_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77385_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77385_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82320_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82320_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 86837_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 86837_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82526_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82526_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82766_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82766_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87879_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87879_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 129248_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 129248_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 197170_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 197170_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 123126_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 123126_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76992_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76992_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 107068_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 107068_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 88515_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 88515_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 92095_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 92095_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 98299_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 98299_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101018_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 101018_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 167326_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 167326_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97921_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97921_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131659_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 131659_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93358_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93358_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91397_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91397_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 96278_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 96278_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104944_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104944_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 124980_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 124980_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 86654_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 86654_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 103324_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 103324_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 93396_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93396_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90174_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 90174_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 183157_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 183157_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 125970_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 125970_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87903_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87903_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 187139_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 187139_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 159959_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 159959_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91732_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91732_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 114244_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 114244_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104310_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104310_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 168877_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 168877_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 196127_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 196127_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 88905_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 88905_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82379_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82379_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91515_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91515_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 116829_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 116829_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 86779_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 86779_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 177052_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 177052_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 157140_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 157140_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115252_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 115252_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104265_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104265_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 88586_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 88586_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 174849_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 174849_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21155_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 21155_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 108838_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 108838_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 94525_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 94525_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91237_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91237_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91375_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91375_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 84356_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 84356_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 94591_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 94591_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 117937_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 117937_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87655_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87655_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 184589_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 184589_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89436_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89436_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 129797_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 129797_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 111415_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 111415_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91016_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91016_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 74404_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74404_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 122894_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 122894_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 73187_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 73187_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:00:44.01 +47:57:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.331 2163973814157582336 315.18263286318 +47.95966521942 13.7624 12.9414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74656_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74656_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 81102_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 81102_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76597_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76597_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 93614_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93614_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89490_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89490_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 126404_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 126404_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 73548_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 73548_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 173368_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 173368_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 109133_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 109133_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89637_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 89637_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:08:45.08 +47:24:08.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 185337_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 185337_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 94806_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 94806_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76478_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76478_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 125714_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 125714_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 169723_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 169723_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78183_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78183_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 181692_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 181692_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 27594_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 27594_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 103759_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 103759_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 165870_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 165870_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 95384_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 95384_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 101306_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 101306_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75416_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75416_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 105463_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 105463_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 186020_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 186020_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 117631_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 117631_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 22257_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 22257_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 86532_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 86532_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 74276_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74276_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97915_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97915_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 122949_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 122949_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 186956_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 186956_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 112354_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 112354_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 81695_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 81695_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75974_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75974_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 166837_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 166837_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76307_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76307_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76808_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76808_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 112688_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 112688_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 199128_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 199128_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75321_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75321_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87588_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87588_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75242_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75242_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 170277_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 170277_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 111122_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 111122_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 93682_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93682_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 51476_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 51476_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:13:56.99 +48:56:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106507_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 106507_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 39792_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 39792_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 216586_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 216586_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:11:37.01 +41:51:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154585_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 154585_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 106891_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 106891_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 171242_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 171242_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 81406_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 81406_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76455_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76455_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 118617_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 118617_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83424_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83424_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 183011_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 183011_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 162549_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 162549_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 172594_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 172594_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82792_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82792_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 146173_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 146173_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 90076_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 90076_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 90377_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 90377_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75164_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75164_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97386_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97386_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77304_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77304_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 114464_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 114464_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76004_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76004_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 74679_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74679_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 112536_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 112536_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91280_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91280_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104504_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104504_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77231_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77231_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 153896_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 153896_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 95573_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 95573_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97233_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97233_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 166302_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 166302_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 183567_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 183567_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82187_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82187_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 86151_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 86151_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87186_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 87186_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 118730_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 118730_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 123877_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 123877_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 195269_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 195269_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76005_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76005_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 93890_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93890_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 79728_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 79728_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 175663_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 175663_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 197006_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 197006_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 101720_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 101720_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 188956_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 188956_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77694_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77694_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 130008_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 130008_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 115495_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 115495_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 94649_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 94649_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89986_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89986_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 199534_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 199534_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 198621_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 198621_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89998_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89998_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77354_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77354_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 80823_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80823_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 186775_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 186775_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82678_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82678_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 111997_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 111997_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83398_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83398_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 90897_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 90897_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 96828_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 96828_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 113205_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 113205_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 84316_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 84316_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91253_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91253_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 119993_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 119993_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 101909_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 101909_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 73499_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 73499_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:02:22.72 +47:58:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.518 2165466233703879680 315.59458329267 +47.97350127235 12.6949 12.2063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106345_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 106345_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 110435_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 110435_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 125457_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 125457_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 190222_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 190222_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 110251_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 110251_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 122837_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 122837_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 173939_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 173939_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75250_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75250_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 111643_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 111643_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 57451_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 57451_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:10:09.84 +48:42:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75987_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75987_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 167979_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 167979_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 100692_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 100692_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 171889_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 171889_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 96728_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 96728_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 96852_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 96852_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78677_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78677_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 80560_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80560_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 96856_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 96856_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 195156_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 195156_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89117_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89117_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 90097_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 90097_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 80938_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80938_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 188037_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 188037_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83192_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83192_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 219522_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 219522_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 101334_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 101334_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 186668_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 186668_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 107611_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 107611_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 174232_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 174232_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 79898_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 79898_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 88623_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 88623_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 132425_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 132425_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 185883_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 185883_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 95515_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 95515_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 176158_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 176158_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76994_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76994_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82420_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82420_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 94336_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 94336_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 105339_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 105339_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 80184_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80184_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 175089_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 175089_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 95853_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 95853_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 184727_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 184727_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 226431_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 226431_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 114397_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 114397_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 91485_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 91485_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 79052_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 79052_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 125769_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 125769_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 88866_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 88866_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 172573_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 172573_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 100809_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 100809_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 191206_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 191206_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 175284_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 175284_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 185025_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 185025_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 195919_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 195919_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97426_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97426_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 116441_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 116441_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 74842_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74842_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 122505_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 122505_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89861_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89861_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 198650_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 198650_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 66374_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 66374_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 99803_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 99803_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83000_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83000_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 103423_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 103423_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 79894_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 79894_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 178552_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 178552_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76125_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76125_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85667_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85667_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 79091_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 79091_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85496_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85496_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104203_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104203_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 165571_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 165571_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 113253_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 113253_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 57411_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 57411_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 157313_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 157313_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:45:29.20 +44:32:48.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 76480_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76480_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 187111_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 187111_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 98285_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 98285_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75168_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75168_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78099_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78099_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 89575_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 89575_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 93692_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93692_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78710_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78710_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 87775_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 87775_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:00:34.83 +47:23:01.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133820_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 133820_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 185867_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 185867_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 94278_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 94278_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 112469_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 112469_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 169698_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 169698_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104732_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104732_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 73787_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 73787_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 125940_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 125940_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 105951_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 105951_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 241557_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 241557_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 110584_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 110584_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76958_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76958_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104582_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104582_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 117632_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 117632_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 106586_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 106586_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 126032_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 126032_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85965_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85965_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 103189_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 103189_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 163468_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 163468_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 143486_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 143486_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 103246_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 103246_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 241439_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 241439_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 73676_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 73676_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 108723_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 108723_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 79783_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 79783_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 175875_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 175875_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75121_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75121_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 224729_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 224729_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 115749_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 115749_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 132178_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 132178_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83689_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83689_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 132454_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 132454_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76306_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76306_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83032_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83032_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 189147_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 189147_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 225037_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 225037_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83193_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83193_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97686_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97686_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 197472_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 197472_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 173168_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 173168_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78928_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78928_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 106838_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 106838_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 20906_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 20906_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97435_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97435_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 80168_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80168_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 175471_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 175471_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77619_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77619_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 104647_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 104647_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85720_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85720_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 101637_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 101637_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 84423_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 84423_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 240814_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 240814_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:01:57.69 +41:52:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.850 1969567277770972160 315.49060752943 +41.87306720819 13.3014 12.7329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 76925_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76925_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 94710_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 94710_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 96143_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 96143_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83709_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83709_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 240755_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 240755_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 195446_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 195446_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 148229_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 148229_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 222134_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 222134_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 224886_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 224886_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:48:31.35 +42:05:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240680_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 240680_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:00:38.48 +46:03:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.511 2163532158400595584 315.16048706935 +46.05837132648 12.7885 12.4172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90286_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 90286_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82419_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82419_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 108958_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 108958_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 172627_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 172627_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85123_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85123_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79372_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 79372_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 171705_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 171705_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 187096_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 187096_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 121288_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 121288_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240484_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
The candidate 240484_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182 did not pass the final checks
**** FOUND 21:04:34.36 +47:08:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 5.563 2165180871767335936 316.14091514439 +47.13926197162 12.6267 11.8061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77802_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77802_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83023_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83023_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27155_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 27155_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 195655_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 195655_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76961_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76961_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85970_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85970_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 169091_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 169091_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88614_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 88614_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98339_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 98339_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179864_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 179864_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 34247_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 34247_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 198462_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 198462_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194724_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 194724_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92369_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 92369_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112101_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 112101_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76834_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76834_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 158095_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 158095_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80969_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80969_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93998_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93998_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80525_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80525_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93968_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 93968_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80488_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80488_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 83807_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 83807_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 80596_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 80596_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 101603_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 101603_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 85327_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 85327_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109619_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 109619_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 192342_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 192342_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 121533_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 121533_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 173597_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 173597_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 106304_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 106304_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97167_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97167_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97710_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97710_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 122229_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 122229_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77817_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77817_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 73633_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 73633_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 134934_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 134934_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 110483_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 110483_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 77946_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 77946_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 82557_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 82557_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 92575_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 92575_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 169831_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 169831_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 75434_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 75434_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 22544_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 22544_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 198540_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 198540_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 22950_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 22950_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 88328_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 88328_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 76796_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 76796_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 84501_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 84501_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 74221_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 74221_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 78982_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 78982_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 172422_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 172422_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 81236_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 81236_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 97342_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 97342_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 179898_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 179898_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 73630_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 73630_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
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Considering the candidate 110899_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
Preparing report for the candidate 110899_fd_Cyg-04-Q2b1x1_2026-03-25_05-56-04_20.00sec_-15.00C_LIGHT_0182
make_report_in_HTML.sh Phase 2 (HTML assembly): 108s
make_report_in_HTML.sh TOTAL: 721s
Prepared the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
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21:58:44.28 +46:55:38.0
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21:04:02.74 +47:01:40.7
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21:00:45.23 +46:59:42.9
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21:00:22.20 +46:58:48.4
21:02:43.22 +46:59:46.5
21:00:49.09 +46:58:36.9
21:00:58.52 +46:58:58.6
21:01:13.23 +46:58:38.3
21:01:19.42 +46:58:50.7
21:01:26.19 +46:58:32.2
21:00:23.24 +46:57:54.6
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21:00:51.77 +46:57:05.1
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########### Completed Cyg-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:45:29.24 +44:32:48.5
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21:00:51.09 +47:16:30.5
21:43:59.41 +43:25:19.2
21:10:14.90 +48:18:57.5
21:01:45.74 +46:54:02.4
21:02:04.66 +47:33:53.5
21:01:17.95 +46:45:47.3
21:02:46.16 +47:42:36.8
21:39:16.74 +42:26:30.7
21:03:33.87 +47:53:01.8
21:02:57.53 +47:28:31.1
21:00:43.49 +47:43:24.8
21:03:46.68 +47:28:32.4
21:02:56.66 +46:45:03.2
21:46:20.28 +44:04:46.1
21:02:03.42 +46:24:30.7
21:10:33.02 +48:40:56.5
21:01:58.90 +47:51:02.7
21:40:58.96 +42:53:16.0
21:00:51.77 +46:57:05.1
21:01:24.12 +47:53:37.8
21:00:24.83 +47:45:31.2
21:00:15.24 +47:16:52.5
21:01:01.04 +47:07:14.8
21:03:11.47 +47:45:34.0
21:01:21.88 +45:36:50.8
21:41:16.45 +42:46:22.6
21:02:13.39 +47:06:48.4
21:00:57.59 +46:25:05.4
21:02:45.85 +44:01:19.2
21:02:29.02 +46:43:18.5
21:01:42.63 +47:57:46.5
21:02:17.05 +45:55:58.5
21:01:17.73 +46:40:29.7
21:00:00.92 +47:54:55.5
21:01:29.17 +46:29:55.8
21:04:43.18 +47:51:03.8
21:00:55.88 +46:42:56.8
21:01:50.57 +46:14:12.1
21:01:18.32 +46:38:44.2
21:01:12.75 +45:54:49.6
21:02:10.79 +47:26:29.8
21:02:34.91 +46:47:04.7
21:46:34.48 +44:10:35.1
21:49:59.36 +45:03:44.4
21:01:10.79 +46:46:08.5
21:00:10.42 +47:56:08.5
21:01:07.13 +46:33:32.6
21:01:00.05 +47:41:38.6
21:44:54.86 +43:34:13.9
21:00:14.05 +47:53:01.5
21:40:48.36 +42:11:06.3
21:00:45.63 +46:17:54.1
21:01:02.34 +45:40:24.0
21:00:20.31 +47:31:07.4
21:01:04.52 +45:39:42.1
21:01:32.66 +47:50:45.8
21:00:12.39 +47:32:58.4
21:41:28.34 +42:57:28.9
21:02:09.12 +42:18:06.5
21:00:20.56 +47:32:40.1
21:01:13.23 +46:58:38.3
21:42:07.74 +43:21:56.0
21:43:01.85 +43:44:28.6
21:01:09.91 +47:44:33.2
21:00:51.08 +46:38:28.1
22:10:52.94 +49:38:37.7
21:00:58.52 +46:58:58.6
21:00:16.81 +47:41:00.9
21:01:46.38 +43:42:50.7
21:04:18.36 +47:48:57.0
21:03:25.10 +46:44:04.1
21:02:57.56 +47:27:45.7
21:00:52.11 +46:49:27.3
21:00:45.51 +47:30:06.6
21:01:04.72 +47:48:55.0
21:01:23.37 +47:05:14.4
21:02:36.73 +47:02:34.5
21:02:38.80 +47:33:01.7
21:00:06.21 +47:39:07.4
21:42:18.50 +43:17:39.2
21:48:27.62 +44:51:17.4
21:03:39.39 +42:08:18.3
21:01:23.78 +47:15:38.4
21:00:20.53 +47:35:01.6
21:00:30.78 +46:33:01.4
21:45:19.54 +43:43:55.8
21:02:45.20 +47:29:25.4
21:01:07.55 +47:42:54.5
21:46:50.91 +43:45:47.6
21:01:42.57 +42:56:49.8
21:00:53.18 +46:05:45.8
21:00:33.77 +47:46:33.7
21:02:22.01 +47:34:49.1
22:09:29.70 +49:22:38.6
21:02:07.48 +43:22:28.0
21:00:40.04 +47:48:49.8
21:00:58.41 +47:25:47.5
21:44:41.77 +43:56:20.6
21:01:03.89 +47:20:01.0
21:00:34.61 +46:56:48.7
21:41:42.49 +42:28:26.3
22:06:51.26 +49:07:03.3
21:41:42.58 +43:28:15.8
21:42:55.45 +43:13:24.3
21:01:20.96 +47:10:44.2
21:02:45.62 +46:26:49.9
21:03:40.21 +47:51:05.9
21:46:00.54 +44:26:43.7
21:03:44.95 +47:40:16.8
21:01:59.98 +47:07:19.4
21:00:17.91 +47:39:14.5
21:01:36.54 +47:07:10.9
21:03:14.96 +47:40:60.0
21:01:10.40 +47:31:34.0
21:01:16.29 +47:39:54.8
21:01:05.42 +46:49:26.4
21:01:48.86 +47:27:56.4
21:01:40.49 +46:31:53.7
21:42:35.88 +43:06:07.4
21:01:42.60 +46:05:33.5
21:46:10.62 +43:40:56.1
21:01:17.70 +46:39:32.3
21:02:46.06 +47:00:34.9
21:01:19.42 +46:58:50.7
21:56:55.68 +45:48:32.0
21:00:26.30 +47:45:58.8
21:00:29.52 +47:56:56.5
21:35:38.64 +45:34:17.4
21:00:48.99 +46:29:42.1
21:01:11.38 +47:47:18.4
21:03:08.72 +47:36:12.4
21:01:08.77 +47:09:53.6
21:02:00.34 +44:02:06.9
21:00:29.82 +47:52:19.3
22:12:06.72 +49:32:35.2
21:46:41.09 +43:22:37.1
22:09:11.03 +49:35:48.1
21:01:14.98 +47:20:40.5
21:00:39.55 +47:49:42.1
21:00:24.76 +47:29:12.8
21:03:43.86 +47:57:01.8
21:01:32.17 +47:44:22.2
21:02:53.71 +43:52:57.2
21:02:30.15 +47:38:53.2
21:00:22.20 +46:58:48.4
21:40:57.21 +42:29:09.1
21:00:06.14 +47:56:10.5
21:00:33.85 +46:28:25.5
###################################################################################
21:45:29.24 +44:32:48.5 -- not an asteroid (will add it to exclusion list)
21:00:49.41 +47:42:57.7 -- not an asteroid (will add it to exclusion list)
21:00:34.83 +47:23:01.6 -- not an asteroid (will add it to exclusion list)
21:01:04.14 +47:53:15.6 -- not an asteroid (will add it to exclusion list)
21:00:36.46 +47:54:44.4 -- not an asteroid (will add it to exclusion list)
21:41:56.50 +43:29:18.8 -- not an asteroid (will add it to exclusion list)
21:08:45.05 +47:24:08.6 -- not an asteroid (will add it to exclusion list)
21:00:33.37 +47:29:25.6 -- not an asteroid (will add it to exclusion list)
21:11:30.25 +45:06:16.2 -- not an asteroid (will add it to exclusion list)
21:10:53.92 +47:22:42.5 -- not an asteroid (will add it to exclusion list)
21:00:44.45 +46:06:59.7 -- not an asteroid (will add it to exclusion list)
21:01:18.55 +46:41:12.8 -- not an asteroid (will add it to exclusion list)
21:01:54.64 +42:42:36.2 -- not an asteroid (will add it to exclusion list)
21:01:46.19 +46:09:51.8 -- not an asteroid (will add it to exclusion list)
21:01:50.41 +47:55:02.9 -- not an asteroid (will add it to exclusion list)
21:10:08.42 +48:51:33.8 -- not an asteroid (will add it to exclusion list)
21:01:38.41 +46:18:07.8 -- not an asteroid (will add it to exclusion list)
21:39:28.77 +42:04:37.6 -- not an asteroid (will add it to exclusion list)
21:02:04.36 +43:52:52.1 -- not an asteroid (will add it to exclusion list)
21:00:24.54 +47:27:40.6 -- not an asteroid (will add it to exclusion list)
21:02:33.31 +46:38:50.7 -- not an asteroid (will add it to exclusion list)
21:58:56.55 +43:22:56.1 -- not an asteroid (will add it to exclusion list)
21:41:38.76 +42:32:27.2 -- not an asteroid (will add it to exclusion list)
21:00:44.11 +46:15:56.8 -- not an asteroid (will add it to exclusion list)
21:43:31.19 +43:06:41.4 -- not an asteroid (will add it to exclusion list)
21:44:45.84 +43:28:19.3 -- not an asteroid (will add it to exclusion list)
21:01:11.17 +46:11:52.3 -- not an asteroid (will add it to exclusion list)
21:00:16.89 +47:16:05.1 -- not an asteroid (will add it to exclusion list)
22:07:50.22 +48:57:43.0 -- not an asteroid (will add it to exclusion list)
21:04:49.68 +44:12:50.6 -- not an asteroid (will add it to exclusion list)
21:02:18.90 +47:12:14.3 -- not an asteroid (will add it to exclusion list)
21:00:42.01 +46:29:12.5 -- not an asteroid (will add it to exclusion list)
21:01:26.19 +46:58:32.2 -- not an asteroid (will add it to exclusion list)
22:12:21.99 +49:22:24.0 -- not an asteroid (will add it to exclusion list)
21:01:27.70 +47:17:20.1 -- not an asteroid (will add it to exclusion list)
21:01:27.53 +47:21:36.3 -- not an asteroid (will add it to exclusion list)
21:00:31.68 +47:20:36.3 -- not an asteroid (will add it to exclusion list)
21:01:21.65 +47:02:22.6 -- not an asteroid (will add it to exclusion list)
21:03:12.16 +43:19:50.4 -- not an asteroid (will add it to exclusion list)
21:00:35.25 +47:07:08.6 -- not an asteroid (will add it to exclusion list)
21:03:50.43 +47:55:38.6 -- not an asteroid (will add it to exclusion list)
21:00:45.23 +46:59:42.9 -- not an asteroid (will add it to exclusion list)
21:43:18.98 +43:57:57.5 -- not an asteroid (will add it to exclusion list)
21:01:10.16 +46:21:53.8 -- not an asteroid (will add it to exclusion list)
21:04:25.79 +44:12:40.7 -- not an asteroid (will add it to exclusion list)
21:00:39.72 +47:21:26.7 -- not an asteroid (will add it to exclusion list)
21:02:48.65 +47:30:14.0 -- not an asteroid (will add it to exclusion list)
21:41:17.27 +43:12:56.5 -- not an asteroid (will add it to exclusion list)
21:01:45.98 +44:02:42.1 -- not an asteroid (will add it to exclusion list)
21:40:51.65 +43:04:31.4 -- not an asteroid (will add it to exclusion list)
21:01:38.07 +43:06:18.6 -- not an asteroid (will add it to exclusion list)
21:01:04.56 +46:16:22.9 -- not an asteroid (will add it to exclusion list)
22:06:55.12 +48:46:16.3 -- not an asteroid (will add it to exclusion list)
21:46:46.23 +44:12:42.3 -- not an asteroid (will add it to exclusion list)
21:06:52.19 +43:27:55.1 -- not an asteroid (will add it to exclusion list)
21:45:37.38 +44:29:47.5 -- not an asteroid (will add it to exclusion list)
21:00:20.58 +47:45:34.2 -- not an asteroid (will add it to exclusion list)
21:01:56.64 +46:52:04.3 -- not an asteroid (will add it to exclusion list)
21:46:01.76 +43:46:35.9 -- not an asteroid (will add it to exclusion list)
21:02:23.13 +47:46:41.1 -- not an asteroid (will add it to exclusion list)
21:00:37.18 +47:50:17.6 -- not an asteroid (will add it to exclusion list)
21:01:22.53 +46:40:19.8 -- not an asteroid (will add it to exclusion list)
21:44:15.59 +43:58:12.3 -- not an asteroid (will add it to exclusion list)
21:01:39.93 +43:55:06.2 -- not an asteroid (will add it to exclusion list)
21:02:03.65 +47:07:10.0 -- not an asteroid (will add it to exclusion list)
21:00:55.95 +47:31:10.3 -- not an asteroid (will add it to exclusion list)
21:01:05.78 +47:40:22.0 -- not an asteroid (will add it to exclusion list)
21:00:08.77 +47:34:15.5 -- not an asteroid (will add it to exclusion list)
21:01:24.29 +47:48:25.7 -- not an asteroid (will add it to exclusion list)
21:00:46.59 +47:34:58.1 -- not an asteroid (will add it to exclusion list)
21:00:41.62 +47:23:33.7 -- not an asteroid (will add it to exclusion list)
21:01:36.59 +47:34:59.8 -- not an asteroid (will add it to exclusion list)
21:01:01.14 +47:34:18.5 -- not an asteroid (will add it to exclusion list)
21:00:24.57 +47:20:44.2 -- not an asteroid (will add it to exclusion list)
21:00:56.58 +45:47:09.1 -- not an asteroid (will add it to exclusion list)
21:01:45.91 +43:27:30.6 -- not an asteroid (will add it to exclusion list)
21:01:32.15 +46:02:08.2 -- not an asteroid (will add it to exclusion list)
21:01:01.95 +47:48:45.1 -- not an asteroid (will add it to exclusion list)
21:01:51.97 +46:37:43.6 -- not an asteroid (will add it to exclusion list)
21:00:43.92 +47:19:26.9 -- not an asteroid (will add it to exclusion list)
21:02:22.54 +47:12:04.9 -- not an asteroid (will add it to exclusion list)
21:03:21.25 +46:58:15.0 -- not an asteroid (will add it to exclusion list)
21:01:25.22 +46:51:10.3 -- not an asteroid (will add it to exclusion list)
21:45:20.75 +44:00:03.1 -- not an asteroid (will add it to exclusion list)
21:01:12.60 +46:58:06.7 -- not an asteroid (will add it to exclusion list)
21:00:46.75 +45:41:15.1 -- not an asteroid (will add it to exclusion list)
21:02:09.50 +47:08:39.4 -- not an asteroid (will add it to exclusion list)
21:01:32.39 +47:13:17.3 -- not an asteroid (will add it to exclusion list)
21:00:32.39 +47:01:19.4 -- not an asteroid (will add it to exclusion list)
21:01:27.88 +46:42:29.0 -- not an asteroid (will add it to exclusion list)
21:01:02.48 +45:57:30.3 -- not an asteroid (will add it to exclusion list)
21:02:15.01 +47:25:04.4 -- not an asteroid (will add it to exclusion list)
21:02:52.24 +46:46:50.6 -- not an asteroid (will add it to exclusion list)
21:03:13.44 +47:09:13.3 -- not an asteroid (will add it to exclusion list)
21:01:11.17 +47:15:47.2 -- not an asteroid (will add it to exclusion list)
21:43:13.11 +42:38:46.9 -- not an asteroid (will add it to exclusion list)
21:01:01.71 +45:55:07.6 -- not an asteroid (will add it to exclusion list)
21:01:51.20 +47:22:01.5 -- not an asteroid (will add it to exclusion list)
21:43:18.09 +42:50:50.1 -- not an asteroid (will add it to exclusion list)
21:03:11.28 +44:29:58.6 -- not an asteroid (will add it to exclusion list)
21:00:27.86 +47:11:35.8 -- not an asteroid (will add it to exclusion list)
21:01:56.03 +46:21:42.6 -- not an asteroid (will add it to exclusion list)
21:03:30.15 +46:45:00.1 -- not an asteroid (will add it to exclusion list)
21:45:07.04 +43:56:01.9 -- not an asteroid (will add it to exclusion list)
21:44:16.56 +43:16:44.0 -- not an asteroid (will add it to exclusion list)
21:00:18.71 +47:17:58.3 -- not an asteroid (will add it to exclusion list)
21:01:59.88 +47:36:05.9 -- not an asteroid (will add it to exclusion list)
21:00:49.27 +47:13:06.5 -- not an asteroid (will add it to exclusion list)
21:01:30.61 +46:16:02.9 -- not an asteroid (will add it to exclusion list)
21:01:35.28 +47:24:12.4 -- not an asteroid (will add it to exclusion list)
21:43:21.11 +43:32:30.7 -- not an asteroid (will add it to exclusion list)
21:46:57.85 +44:28:25.6 -- not an asteroid (will add it to exclusion list)
21:01:22.16 +46:19:21.6 -- not an asteroid (will add it to exclusion list)
21:01:58.11 +46:44:17.8 -- not an asteroid (will add it to exclusion list)
21:01:45.71 +47:20:23.6 -- not an asteroid (will add it to exclusion list)
21:44:37.00 +43:37:40.5 -- not an asteroid (will add it to exclusion list)
22:12:11.13 +49:35:54.6 -- not an asteroid (will add it to exclusion list)
21:01:40.40 +46:34:08.0 -- not an asteroid (will add it to exclusion list)
21:01:21.15 +47:05:57.4 -- not an asteroid (will add it to exclusion list)
21:02:53.33 +47:14:25.7 -- not an asteroid (will add it to exclusion list)
21:01:15.69 +47:12:56.9 -- not an asteroid (will add it to exclusion list)
21:00:21.50 +47:29:48.5 -- not an asteroid (will add it to exclusion list)
21:00:26.69 +47:04:58.5 -- not an asteroid (will add it to exclusion list)
21:00:36.25 +46:12:48.1 -- not an asteroid (will add it to exclusion list)
21:01:38.56 +47:22:15.5 -- not an asteroid (will add it to exclusion list)
21:02:22.22 +42:50:31.9 -- not an asteroid (will add it to exclusion list)
21:03:16.95 +47:18:56.9 -- not an asteroid (will add it to exclusion list)
21:01:26.14 +45:46:14.3 -- not an asteroid (will add it to exclusion list)
21:01:11.44 +46:27:37.4 -- not an asteroid (will add it to exclusion list)
21:00:39.36 +47:14:04.7 -- not an asteroid (will add it to exclusion list)
21:00:12.04 +47:54:15.9 -- not an asteroid (will add it to exclusion list)
21:01:33.79 +46:02:45.1 -- not an asteroid (will add it to exclusion list)
21:00:50.61 +47:55:23.3 -- not an asteroid (will add it to exclusion list)
21:00:52.66 +47:40:07.2 -- not an asteroid (will add it to exclusion list)
21:03:12.89 +47:51:12.9 -- not an asteroid (will add it to exclusion list)
21:02:56.12 +47:08:25.4 -- not an asteroid (will add it to exclusion list)
21:00:26.99 +47:16:52.7 -- not an asteroid (will add it to exclusion list)
21:01:46.70 +45:54:21.4 -- not an asteroid (will add it to exclusion list)
21:01:15.94 +47:57:35.1 -- not an asteroid (will add it to exclusion list)
21:44:48.67 +43:42:11.4 -- not an asteroid (will add it to exclusion list)
21:01:19.24 +46:32:51.4 -- not an asteroid (will add it to exclusion list)
21:41:55.36 +42:45:07.1 -- not an asteroid (will add it to exclusion list)
21:02:34.58 +47:05:41.7 -- not an asteroid (will add it to exclusion list)
21:03:20.15 +47:52:05.2 -- not an asteroid (will add it to exclusion list)
21:01:06.83 +45:55:39.0 -- not an asteroid (will add it to exclusion list)
21:44:41.65 +43:53:38.5 -- not an asteroid (will add it to exclusion list)
21:00:56.64 +47:45:39.5 -- not an asteroid (will add it to exclusion list)
21:41:07.22 +42:35:09.6 -- not an asteroid (will add it to exclusion list)
22:09:01.64 +49:22:14.8 -- not an asteroid (will add it to exclusion list)
21:01:17.60 +46:44:42.6 -- not an asteroid (will add it to exclusion list)
21:47:17.98 +44:02:39.3 -- not an asteroid (will add it to exclusion list)
21:01:57.15 +47:04:09.8 -- not an asteroid (will add it to exclusion list)
21:00:31.27 +46:49:47.5 -- not an asteroid (will add it to exclusion list)
21:03:44.81 +47:54:42.4 -- not an asteroid (will add it to exclusion list)
21:02:27.96 +46:42:00.0 -- not an asteroid (will add it to exclusion list)
21:40:11.37 +42:48:51.6 -- not an asteroid (will add it to exclusion list)
21:01:54.84 +46:14:13.6 -- not an asteroid (will add it to exclusion list)
22:11:04.37 +49:35:08.6 -- not an asteroid (will add it to exclusion list)
21:01:46.97 +47:25:14.5 -- not an asteroid (will add it to exclusion list)
21:04:25.45 +47:57:28.0 -- not an asteroid (will add it to exclusion list)
21:00:23.24 +46:57:54.6 -- not an asteroid (will add it to exclusion list)
21:01:48.44 +46:02:22.3 -- not an asteroid (will add it to exclusion list)
21:42:28.79 +42:49:49.7 -- not an asteroid (will add it to exclusion list)
21:01:56.76 +46:26:30.0 -- not an asteroid (will add it to exclusion list)
21:02:52.14 +47:37:54.6 -- not an asteroid (will add it to exclusion list)
21:02:58.76 +47:52:40.4 -- not an asteroid (will add it to exclusion list)
21:45:40.24 +44:01:21.8 -- not an asteroid (will add it to exclusion list)
21:00:44.06 +47:50:17.9 -- not an asteroid (will add it to exclusion list)
21:01:06.42 +47:49:44.7 -- not an asteroid (will add it to exclusion list)
21:02:14.94 +46:25:35.7 -- not an asteroid (will add it to exclusion list)
21:45:21.29 +43:25:05.6 -- not an asteroid (will add it to exclusion list)
21:00:59.22 +47:53:10.6 -- not an asteroid (will add it to exclusion list)
21:01:15.87 +47:22:29.0 -- not an asteroid (will add it to exclusion list)
21:03:15.41 +47:54:39.8 -- not an asteroid (will add it to exclusion list)
21:46:26.80 +43:50:35.2 -- not an asteroid (will add it to exclusion list)
21:01:29.37 +46:29:00.9 -- not an asteroid (will add it to exclusion list)
21:00:47.85 +47:07:24.2 -- not an asteroid (will add it to exclusion list)
21:02:07.28 +46:39:22.5 -- not an asteroid (will add it to exclusion list)
22:07:19.91 +48:50:45.8 -- not an asteroid (will add it to exclusion list)
21:47:08.06 +44:35:10.4 -- not an asteroid (will add it to exclusion list)
21:01:19.74 +46:38:16.3 -- not an asteroid (will add it to exclusion list)
21:44:37.68 +43:49:23.1 -- not an asteroid (will add it to exclusion list)
21:03:25.89 +47:38:60.0 -- not an asteroid (will add it to exclusion list)
21:00:07.72 +47:50:00.1 -- not an asteroid (will add it to exclusion list)
21:01:29.04 +46:11:49.8 -- not an asteroid (will add it to exclusion list)
21:00:24.64 +47:32:02.6 -- not an asteroid (will add it to exclusion list)
21:01:47.69 +42:44:55.1 -- not an asteroid (will add it to exclusion list)
21:43:55.89 +44:15:44.6 -- not an asteroid (will add it to exclusion list)
21:45:47.46 +43:43:38.4 -- not an asteroid (will add it to exclusion list)
21:01:07.74 +47:34:38.7 -- not an asteroid (will add it to exclusion list)
21:48:36.69 +44:56:50.0 -- not an asteroid (will add it to exclusion list)
21:02:12.13 +47:16:49.6 -- not an asteroid (will add it to exclusion list)
21:58:44.28 +46:55:38.0 -- not an asteroid (will add it to exclusion list)
21:00:11.76 +47:53:24.2 -- not an asteroid (will add it to exclusion list)
21:02:43.22 +46:59:46.5 -- not an asteroid (will add it to exclusion list)
21:03:42.43 +47:50:10.8 -- not an asteroid (will add it to exclusion list)
21:01:24.45 +46:22:15.9 -- not an asteroid (will add it to exclusion list)
21:01:01.46 +47:51:41.2 -- not an asteroid (will add it to exclusion list)
21:00:46.35 +47:54:14.8 -- not an asteroid (will add it to exclusion list)
21:00:36.27 +46:25:02.5 -- not an asteroid (will add it to exclusion list)
21:00:16.88 +47:12:34.7 -- not an asteroid (will add it to exclusion list)
21:01:36.59 +46:43:18.2 -- not an asteroid (will add it to exclusion list)
21:04:04.48 +47:50:17.6 -- not an asteroid (will add it to exclusion list)
21:45:01.30 +44:39:16.3 -- not an asteroid (will add it to exclusion list)
21:00:35.54 +47:02:37.3 -- not an asteroid (will add it to exclusion list)
21:02:27.46 +47:00:00.9 -- not an asteroid (will add it to exclusion list)
21:47:12.83 +44:01:35.8 -- not an asteroid (will add it to exclusion list)
21:01:53.32 +42:46:25.5 -- not an asteroid (will add it to exclusion list)
21:02:15.11 +47:36:31.5 -- not an asteroid (will add it to exclusion list)
21:01:07.81 +47:25:27.1 -- not an asteroid (will add it to exclusion list)
21:01:45.94 +47:23:15.0 -- not an asteroid (will add it to exclusion list)
21:01:33.41 +46:11:37.4 -- not an asteroid (will add it to exclusion list)
21:01:55.93 +46:00:20.1 -- not an asteroid (will add it to exclusion list)
21:50:37.88 +43:08:50.2 -- not an asteroid (will add it to exclusion list)
21:03:43.22 +47:52:40.9 -- not an asteroid (will add it to exclusion list)
21:00:35.49 +47:06:30.4 -- not an asteroid (will add it to exclusion list)
21:01:51.62 +47:43:23.7 -- not an asteroid (will add it to exclusion list)
21:43:14.65 +43:36:25.3 -- not an asteroid (will add it to exclusion list)
21:01:37.03 +43:27:40.2 -- not an asteroid (will add it to exclusion list)
21:52:49.64 +46:37:11.7 -- not an asteroid (will add it to exclusion list)
21:36:17.87 +43:02:43.0 -- not an asteroid (will add it to exclusion list)
21:00:26.73 +47:46:46.9 -- not an asteroid (will add it to exclusion list)
21:01:44.25 +45:45:58.0 -- not an asteroid (will add it to exclusion list)
21:01:09.22 +46:18:42.9 -- not an asteroid (will add it to exclusion list)
21:02:14.83 +47:06:29.7 -- not an asteroid (will add it to exclusion list)
21:01:19.61 +47:16:27.8 -- not an asteroid (will add it to exclusion list)
21:01:34.86 +43:35:54.5 -- not an asteroid (will add it to exclusion list)
21:44:27.49 +43:26:11.4 -- not an asteroid (will add it to exclusion list)
21:02:41.13 +47:17:01.0 -- not an asteroid (will add it to exclusion list)
21:00:25.41 +47:47:45.1 -- not an asteroid (will add it to exclusion list)
21:01:08.50 +47:39:27.5 -- not an asteroid (will add it to exclusion list)
21:42:28.69 +42:50:57.8 -- not an asteroid (will add it to exclusion list)
21:01:11.25 +47:34:36.1 -- not an asteroid (will add it to exclusion list)
21:00:48.90 +46:26:08.0 -- not an asteroid (will add it to exclusion list)
21:02:52.62 +47:33:34.2 -- not an asteroid (will add it to exclusion list)
21:00:49.47 +47:13:47.2 -- not an asteroid (will add it to exclusion list)
21:02:49.04 +47:01:18.2 -- not an asteroid (will add it to exclusion list)
21:02:10.08 +46:24:26.4 -- not an asteroid (will add it to exclusion list)
21:01:22.56 +47:30:32.2 -- not an asteroid (will add it to exclusion list)
21:01:42.77 +47:15:05.6 -- not an asteroid (will add it to exclusion list)
21:02:09.60 +46:09:28.1 -- not an asteroid (will add it to exclusion list)
21:00:28.29 +46:48:39.2 -- not an asteroid (will add it to exclusion list)
21:02:05.91 +46:40:05.4 -- not an asteroid (will add it to exclusion list)
21:02:36.53 +46:30:50.2 -- not an asteroid (will add it to exclusion list)
21:01:45.06 +45:56:35.4 -- not an asteroid (will add it to exclusion list)
21:02:47.34 +43:03:31.5 -- not an asteroid (will add it to exclusion list)
21:01:01.67 +46:30:17.8 -- not an asteroid (will add it to exclusion list)
21:01:07.73 +46:02:12.6 -- not an asteroid (will add it to exclusion list)
21:02:57.65 +43:48:19.2 -- not an asteroid (will add it to exclusion list)
21:01:12.66 +47:53:16.1 -- not an asteroid (will add it to exclusion list)
21:00:49.12 +46:27:02.3 -- not an asteroid (will add it to exclusion list)
21:00:21.45 +47:50:50.7 -- not an asteroid (will add it to exclusion list)
21:46:31.69 +43:57:33.9 -- not an asteroid (will add it to exclusion list)
21:00:24.71 +46:51:21.6 -- not an asteroid (will add it to exclusion list)
21:37:14.43 +43:52:38.5 -- not an asteroid (will add it to exclusion list)
21:00:58.49 +47:00:10.6 -- not an asteroid (will add it to exclusion list)
21:04:02.74 +47:01:40.7 -- not an asteroid (will add it to exclusion list)
21:00:51.95 +47:44:30.1 -- not an asteroid (will add it to exclusion list)
21:00:19.63 +47:39:08.7 -- not an asteroid (will add it to exclusion list)
21:02:25.44 +47:00:50.4 -- not an asteroid (will add it to exclusion list)
21:42:13.13 +43:16:50.4 -- not an asteroid (will add it to exclusion list)
21:01:33.44 +47:18:42.9 -- not an asteroid (will add it to exclusion list)
21:00:16.39 +47:15:21.2 -- not an asteroid (will add it to exclusion list)
21:02:50.98 +47:39:38.5 -- not an asteroid (will add it to exclusion list)
21:41:11.13 +42:55:31.4 -- not an asteroid (will add it to exclusion list)
21:00:52.61 +47:33:02.8 -- not an asteroid (will add it to exclusion list)
21:02:33.13 +41:55:25.8 -- not an asteroid (will add it to exclusion list)
21:01:31.06 +46:50:45.4 -- not an asteroid (will add it to exclusion list)
21:43:28.59 +42:48:18.0 -- not an asteroid (will add it to exclusion list)
21:00:28.66 +46:35:37.0 -- not an asteroid (will add it to exclusion list)
21:43:35.41 +43:40:39.7 -- not an asteroid (will add it to exclusion list)
21:02:29.34 +47:42:30.7 -- not an asteroid (will add it to exclusion list)
21:00:48.71 +47:19:28.6 -- not an asteroid (will add it to exclusion list)
21:01:08.44 +45:39:36.1 -- not an asteroid (will add it to exclusion list)
21:44:30.99 +42:43:17.8 -- not an asteroid (will add it to exclusion list)
21:01:44.34 +47:03:38.9 -- not an asteroid (will add it to exclusion list)
21:02:05.80 +43:40:49.4 -- not an asteroid (will add it to exclusion list)
21:00:39.39 +47:48:27.1 -- not an asteroid (will add it to exclusion list)
21:01:53.80 +47:35:41.1 -- not an asteroid (will add it to exclusion list)
21:01:03.33 +47:06:17.9 -- not an asteroid (will add it to exclusion list)
21:00:56.50 +46:41:10.3 -- not an asteroid (will add it to exclusion list)
21:02:19.26 +47:41:50.1 -- not an asteroid (will add it to exclusion list)
21:43:38.89 +43:37:42.6 -- not an asteroid (will add it to exclusion list)
21:01:55.27 +47:03:18.7 -- not an asteroid (will add it to exclusion list)
21:03:52.08 +42:49:39.7 -- not an asteroid (will add it to exclusion list)
21:02:23.53 +42:21:57.0 -- not an asteroid (will add it to exclusion list)
21:01:45.40 +46:21:17.7 -- not an asteroid (will add it to exclusion list)
21:00:36.95 +47:12:33.2 -- not an asteroid (will add it to exclusion list)
21:00:24.33 +47:43:19.3 -- not an asteroid (will add it to exclusion list)
21:01:39.88 +45:56:16.0 -- not an asteroid (will add it to exclusion list)
21:02:04.89 +47:19:57.6 -- not an asteroid (will add it to exclusion list)
21:46:13.65 +43:43:19.4 -- not an asteroid (will add it to exclusion list)
21:02:04.87 +46:52:03.5 -- not an asteroid (will add it to exclusion list)
21:03:53.32 +43:09:58.8 -- not an asteroid (will add it to exclusion list)
21:45:23.45 +43:35:34.9 -- not an asteroid (will add it to exclusion list)
21:02:19.73 +42:51:14.0 -- not an asteroid (will add it to exclusion list)
21:42:38.34 +43:18:23.7 -- not an asteroid (will add it to exclusion list)
21:00:49.09 +46:58:36.9 -- not an asteroid (will add it to exclusion list)
21:01:43.22 +46:17:05.5 -- not an asteroid (will add it to exclusion list)
21:00:54.20 +47:54:28.5 -- not an asteroid (will add it to exclusion list)
21:00:48.99 +46:02:47.9 -- not an asteroid (will add it to exclusion list)
21:00:51.09 +47:16:30.5 -- not an asteroid (will add it to exclusion list)
21:43:59.41 +43:25:19.2 -- not an asteroid (will add it to exclusion list)
21:10:14.90 +48:18:57.5 -- not an asteroid (will add it to exclusion list)
21:01:45.74 +46:54:02.4 -- not an asteroid (will add it to exclusion list)
21:02:04.66 +47:33:53.5 -- not an asteroid (will add it to exclusion list)
21:01:17.95 +46:45:47.3 -- not an asteroid (will add it to exclusion list)
21:02:46.16 +47:42:36.8 -- not an asteroid (will add it to exclusion list)
21:39:16.74 +42:26:30.7 -- not an asteroid (will add it to exclusion list)
21:03:33.87 +47:53:01.8 -- not an asteroid (will add it to exclusion list)
21:02:57.53 +47:28:31.1 -- not an asteroid (will add it to exclusion list)
21:00:43.49 +47:43:24.8 -- not an asteroid (will add it to exclusion list)
21:03:46.68 +47:28:32.4 -- not an asteroid (will add it to exclusion list)
21:02:56.66 +46:45:03.2 -- not an asteroid (will add it to exclusion list)
21:46:20.28 +44:04:46.1 -- not an asteroid (will add it to exclusion list)
21:02:03.42 +46:24:30.7 -- not an asteroid (will add it to exclusion list)
21:10:33.02 +48:40:56.5 -- not an asteroid (will add it to exclusion list)
21:01:58.90 +47:51:02.7 -- not an asteroid (will add it to exclusion list)
21:40:58.96 +42:53:16.0 -- not an asteroid (will add it to exclusion list)
21:00:51.77 +46:57:05.1 -- not an asteroid (will add it to exclusion list)
21:01:24.12 +47:53:37.8 -- not an asteroid (will add it to exclusion list)
21:00:24.83 +47:45:31.2 -- not an asteroid (will add it to exclusion list)
21:00:15.24 +47:16:52.5 -- not an asteroid (will add it to exclusion list)
21:01:01.04 +47:07:14.8 -- not an asteroid (will add it to exclusion list)
21:03:11.47 +47:45:34.0 -- not an asteroid (will add it to exclusion list)
21:01:21.88 +45:36:50.8 -- not an asteroid (will add it to exclusion list)
21:41:16.45 +42:46:22.6 -- not an asteroid (will add it to exclusion list)
21:02:13.39 +47:06:48.4 -- not an asteroid (will add it to exclusion list)
21:00:57.59 +46:25:05.4 -- not an asteroid (will add it to exclusion list)
21:02:45.85 +44:01:19.2 -- not an asteroid (will add it to exclusion list)
21:02:29.02 +46:43:18.5 -- not an asteroid (will add it to exclusion list)
21:01:42.63 +47:57:46.5 -- not an asteroid (will add it to exclusion list)
21:02:17.05 +45:55:58.5 -- not an asteroid (will add it to exclusion list)
21:01:17.73 +46:40:29.7 -- not an asteroid (will add it to exclusion list)
21:00:00.92 +47:54:55.5 -- not an asteroid (will add it to exclusion list)
21:01:29.17 +46:29:55.8 -- not an asteroid (will add it to exclusion list)
21:04:43.18 +47:51:03.8 -- not an asteroid (will add it to exclusion list)
21:00:55.88 +46:42:56.8 -- not an asteroid (will add it to exclusion list)
21:01:50.57 +46:14:12.1 -- not an asteroid (will add it to exclusion list)
21:01:18.32 +46:38:44.2 -- not an asteroid (will add it to exclusion list)
21:01:12.75 +45:54:49.6 -- not an asteroid (will add it to exclusion list)
21:02:10.79 +47:26:29.8 -- not an asteroid (will add it to exclusion list)
21:02:34.91 +46:47:04.7 -- not an asteroid (will add it to exclusion list)
21:46:34.48 +44:10:35.1 -- not an asteroid (will add it to exclusion list)
21:49:59.36 +45:03:44.4 -- not an asteroid (will add it to exclusion list)
21:01:10.79 +46:46:08.5 -- not an asteroid (will add it to exclusion list)
21:00:10.42 +47:56:08.5 -- not an asteroid (will add it to exclusion list)
21:01:07.13 +46:33:32.6 -- not an asteroid (will add it to exclusion list)
21:01:00.05 +47:41:38.6 -- not an asteroid (will add it to exclusion list)
21:44:54.86 +43:34:13.9 -- not an asteroid (will add it to exclusion list)
21:00:14.05 +47:53:01.5 -- not an asteroid (will add it to exclusion list)
21:40:48.36 +42:11:06.3 -- not an asteroid (will add it to exclusion list)
21:00:45.63 +46:17:54.1 -- not an asteroid (will add it to exclusion list)
21:01:02.34 +45:40:24.0 -- not an asteroid (will add it to exclusion list)
21:00:20.31 +47:31:07.4 -- not an asteroid (will add it to exclusion list)
21:01:04.52 +45:39:42.1 -- not an asteroid (will add it to exclusion list)
21:01:32.66 +47:50:45.8 -- not an asteroid (will add it to exclusion list)
21:00:12.39 +47:32:58.4 -- not an asteroid (will add it to exclusion list)
21:41:28.34 +42:57:28.9 -- not an asteroid (will add it to exclusion list)
21:02:09.12 +42:18:06.5 -- not an asteroid (will add it to exclusion list)
21:00:20.56 +47:32:40.1 -- not an asteroid (will add it to exclusion list)
21:01:13.23 +46:58:38.3 -- not an asteroid (will add it to exclusion list)
21:42:07.74 +43:21:56.0 -- not an asteroid (will add it to exclusion list)
21:43:01.85 +43:44:28.6 -- not an asteroid (will add it to exclusion list)
21:01:09.91 +47:44:33.2 -- not an asteroid (will add it to exclusion list)
21:00:51.08 +46:38:28.1 -- not an asteroid (will add it to exclusion list)
22:10:52.94 +49:38:37.7 -- not an asteroid (will add it to exclusion list)
21:00:58.52 +46:58:58.6 -- not an asteroid (will add it to exclusion list)
21:00:16.81 +47:41:00.9 -- not an asteroid (will add it to exclusion list)
21:01:46.38 +43:42:50.7 -- not an asteroid (will add it to exclusion list)
21:04:18.36 +47:48:57.0 -- not an asteroid (will add it to exclusion list)
21:03:25.10 +46:44:04.1 -- not an asteroid (will add it to exclusion list)
21:02:57.56 +47:27:45.7 -- not an asteroid (will add it to exclusion list)
21:00:52.11 +46:49:27.3 -- not an asteroid (will add it to exclusion list)
21:00:45.51 +47:30:06.6 -- not an asteroid (will add it to exclusion list)
21:01:04.72 +47:48:55.0 -- not an asteroid (will add it to exclusion list)
21:01:23.37 +47:05:14.4 -- not an asteroid (will add it to exclusion list)
21:02:36.73 +47:02:34.5 -- not an asteroid (will add it to exclusion list)
21:02:38.80 +47:33:01.7 -- not an asteroid (will add it to exclusion list)
21:00:06.21 +47:39:07.4 -- not an asteroid (will add it to exclusion list)
21:42:18.50 +43:17:39.2 -- not an asteroid (will add it to exclusion list)
21:48:27.62 +44:51:17.4 -- not an asteroid (will add it to exclusion list)
21:03:39.39 +42:08:18.3 -- not an asteroid (will add it to exclusion list)
21:01:23.78 +47:15:38.4 -- not an asteroid (will add it to exclusion list)
21:00:20.53 +47:35:01.6 -- not an asteroid (will add it to exclusion list)
21:00:30.78 +46:33:01.4 -- not an asteroid (will add it to exclusion list)
21:45:19.54 +43:43:55.8 -- not an asteroid (will add it to exclusion list)
21:02:45.20 +47:29:25.4 -- not an asteroid (will add it to exclusion list)
21:01:07.55 +47:42:54.5 -- not an asteroid (will add it to exclusion list)
21:46:50.91 +43:45:47.6 -- not an asteroid (will add it to exclusion list)
21:01:42.57 +42:56:49.8 -- not an asteroid (will add it to exclusion list)
21:00:53.18 +46:05:45.8 -- not an asteroid (will add it to exclusion list)
21:00:33.77 +47:46:33.7 -- not an asteroid (will add it to exclusion list)
21:02:22.01 +47:34:49.1 -- not an asteroid (will add it to exclusion list)
22:09:29.70 +49:22:38.6 -- not an asteroid (will add it to exclusion list)
21:02:07.48 +43:22:28.0 -- not an asteroid (will add it to exclusion list)
21:00:40.04 +47:48:49.8 -- not an asteroid (will add it to exclusion list)
21:00:58.41 +47:25:47.5 -- not an asteroid (will add it to exclusion list)
21:44:41.77 +43:56:20.6 -- not an asteroid (will add it to exclusion list)
21:01:03.89 +47:20:01.0 -- not an asteroid (will add it to exclusion list)
21:00:34.61 +46:56:48.7 -- not an asteroid (will add it to exclusion list)
21:41:42.49 +42:28:26.3 -- not an asteroid (will add it to exclusion list)
22:06:51.26 +49:07:03.3 -- not an asteroid (will add it to exclusion list)
21:41:42.58 +43:28:15.8 -- not an asteroid (will add it to exclusion list)
21:42:55.45 +43:13:24.3 -- not an asteroid (will add it to exclusion list)
21:01:20.96 +47:10:44.2 -- not an asteroid (will add it to exclusion list)
21:02:45.62 +46:26:49.9 -- not an asteroid (will add it to exclusion list)
21:03:40.21 +47:51:05.9 -- not an asteroid (will add it to exclusion list)
21:46:00.54 +44:26:43.7 -- not an asteroid (will add it to exclusion list)
21:03:44.95 +47:40:16.8 -- not an asteroid (will add it to exclusion list)
21:01:59.98 +47:07:19.4 -- not an asteroid (will add it to exclusion list)
21:00:17.91 +47:39:14.5 -- not an asteroid (will add it to exclusion list)
21:01:36.54 +47:07:10.9 -- not an asteroid (will add it to exclusion list)
21:03:14.96 +47:40:60.0 -- not an asteroid (will add it to exclusion list)
21:01:10.40 +47:31:34.0 -- not an asteroid (will add it to exclusion list)
21:01:16.29 +47:39:54.8 -- not an asteroid (will add it to exclusion list)
21:01:05.42 +46:49:26.4 -- not an asteroid (will add it to exclusion list)
21:01:48.86 +47:27:56.4 -- not an asteroid (will add it to exclusion list)
21:01:40.49 +46:31:53.7 -- not an asteroid (will add it to exclusion list)
21:42:35.88 +43:06:07.4 -- not an asteroid (will add it to exclusion list)
21:01:42.60 +46:05:33.5 -- not an asteroid (will add it to exclusion list)
21:46:10.62 +43:40:56.1 -- not an asteroid (will add it to exclusion list)
21:01:17.70 +46:39:32.3 -- not an asteroid (will add it to exclusion list)
21:02:46.06 +47:00:34.9 -- not an asteroid (will add it to exclusion list)
21:01:19.42 +46:58:50.7 -- not an asteroid (will add it to exclusion list)
21:56:55.68 +45:48:32.0 -- not an asteroid (will add it to exclusion list)
21:00:26.30 +47:45:58.8 -- not an asteroid (will add it to exclusion list)
21:00:29.52 +47:56:56.5 -- not an asteroid (will add it to exclusion list)
21:35:38.64 +45:34:17.4 -- not an asteroid (will add it to exclusion list)
21:00:48.99 +46:29:42.1 -- not an asteroid (will add it to exclusion list)
21:01:11.38 +47:47:18.4 -- not an asteroid (will add it to exclusion list)
21:03:08.72 +47:36:12.4 -- not an asteroid (will add it to exclusion list)
21:01:08.77 +47:09:53.6 -- not an asteroid (will add it to exclusion list)
21:02:00.34 +44:02:06.9 -- not an asteroid (will add it to exclusion list)
21:00:29.82 +47:52:19.3 -- not an asteroid (will add it to exclusion list)
22:12:06.72 +49:32:35.2 -- not an asteroid (will add it to exclusion list)
21:46:41.09 +43:22:37.1 -- not an asteroid (will add it to exclusion list)
22:09:11.03 +49:35:48.1 -- not an asteroid (will add it to exclusion list)
21:01:14.98 +47:20:40.5 -- not an asteroid (will add it to exclusion list)
21:00:39.55 +47:49:42.1 -- not an asteroid (will add it to exclusion list)
21:00:24.76 +47:29:12.8 -- not an asteroid (will add it to exclusion list)
21:03:43.86 +47:57:01.8 -- not an asteroid (will add it to exclusion list)
21:01:32.17 +47:44:22.2 -- not an asteroid (will add it to exclusion list)
21:02:53.71 +43:52:57.2 -- not an asteroid (will add it to exclusion list)
21:02:30.15 +47:38:53.2 -- not an asteroid (will add it to exclusion list)
21:00:22.20 +46:58:48.4 -- not an asteroid (will add it to exclusion list)
21:40:57.21 +42:29:09.1 -- not an asteroid (will add it to exclusion list)
21:00:06.14 +47:56:10.5 -- not an asteroid (will add it to exclusion list)
21:00:33.85 +46:28:25.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:00:00.92 +47:54:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:06.14 +47:56:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:06.21 +47:39:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:07.72 +47:50:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:08.77 +47:34:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:10.42 +47:56:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:11.76 +47:53:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:12.04 +47:54:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:12.39 +47:32:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:14.05 +47:53:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:15.24 +47:16:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:16.39 +47:15:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:16.81 +47:41:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:16.88 +47:12:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:16.89 +47:16:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:17.91 +47:39:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:18.71 +47:17:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:19.63 +47:39:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:20.31 +47:31:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:20.53 +47:35:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:20.56 +47:32:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:20.58 +47:45:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:21.45 +47:50:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:21.50 +47:29:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:22.20 +46:58:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:23.24 +46:57:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:24.33 +47:43:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:24.54 +47:27:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:24.57 +47:20:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:24.64 +47:32:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:24.71 +46:51:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:24.76 +47:29:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:24.83 +47:45:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:25.41 +47:47:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:26.30 +47:45:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:26.69 +47:04:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:26.73 +47:46:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:26.99 +47:16:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:27.86 +47:11:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:28.29 +46:48:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:28.66 +46:35:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:29.52 +47:56:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:29.82 +47:52:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:30.78 +46:33:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:31.27 +46:49:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:31.68 +47:20:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:32.39 +47:01:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:33.37 +47:29:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:33.77 +47:46:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:33.85 +46:28:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:34.61 +46:56:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:34.83 +47:23:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:35.25 +47:07:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:35.49 +47:06:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:35.54 +47:02:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:36.25 +46:12:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:36.27 +46:25:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:36.46 +47:54:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:36.95 +47:12:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:37.18 +47:50:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:39.36 +47:14:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:39.39 +47:48:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:39.55 +47:49:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:39.72 +47:21:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:40.04 +47:48:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:41.62 +47:23:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:42.01 +46:29:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:43.49 +47:43:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:43.92 +47:19:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:44.06 +47:50:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:44.11 +46:15:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:44.45 +46:06:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:45.23 +46:59:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:45.51 +47:30:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:45.63 +46:17:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:46.35 +47:54:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:46.59 +47:34:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:46.75 +45:41:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:47.85 +47:07:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:48.71 +47:19:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:48.90 +46:26:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:48.99 +46:02:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:48.99 +46:29:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:49.09 +46:58:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:49.12 +46:27:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:49.27 +47:13:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:49.41 +47:42:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:49.47 +47:13:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:50.61 +47:55:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:51.08 +46:38:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:51.09 +47:16:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:51.77 +46:57:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:51.95 +47:44:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:52.11 +46:49:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:52.61 +47:33:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:52.66 +47:40:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:53.18 +46:05:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:54.20 +47:54:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:55.88 +46:42:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:55.95 +47:31:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:56.50 +46:41:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:56.58 +45:47:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:56.64 +47:45:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:57.59 +46:25:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:58.41 +47:25:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:58.49 +47:00:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:58.52 +46:58:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:59.22 +47:53:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:00.05 +47:41:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:01.04 +47:07:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:01.14 +47:34:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:01.46 +47:51:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:01.67 +46:30:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:01.71 +45:55:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:01.95 +47:48:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:02.34 +45:40:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:02.48 +45:57:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:03.33 +47:06:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:03.89 +47:20:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:04.14 +47:53:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:04.52 +45:39:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:04.56 +46:16:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:04.72 +47:48:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:05.42 +46:49:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:05.78 +47:40:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:06.42 +47:49:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:06.83 +45:55:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:07.13 +46:33:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:07.55 +47:42:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:07.73 +46:02:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:07.74 +47:34:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:07.81 +47:25:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:08.44 +45:39:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:08.50 +47:39:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:08.77 +47:09:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:09.22 +46:18:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:09.91 +47:44:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:10.16 +46:21:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:10.40 +47:31:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:10.79 +46:46:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:11.17 +46:11:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:11.17 +47:15:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:11.25 +47:34:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:11.38 +47:47:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:11.44 +46:27:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:12.60 +46:58:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:12.66 +47:53:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:12.75 +45:54:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:13.23 +46:58:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:14.98 +47:20:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:15.69 +47:12:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:15.87 +47:22:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:15.94 +47:57:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:16.29 +47:39:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:17.60 +46:44:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:17.70 +46:39:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:17.73 +46:40:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:17.95 +46:45:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:18.32 +46:38:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:18.55 +46:41:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:19.24 +46:32:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:19.42 +46:58:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:19.61 +47:16:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:19.74 +46:38:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:20.96 +47:10:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:21.15 +47:05:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:21.65 +47:02:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:21.88 +45:36:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:22.16 +46:19:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:22.53 +46:40:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:22.56 +47:30:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:23.37 +47:05:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:23.78 +47:15:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:24.12 +47:53:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:24.29 +47:48:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:24.45 +46:22:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:25.22 +46:51:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:26.14 +45:46:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:26.19 +46:58:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:27.53 +47:21:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:27.70 +47:17:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:27.88 +46:42:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:29.04 +46:11:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:29.17 +46:29:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:29.37 +46:29:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:30.61 +46:16:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:31.06 +46:50:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:32.15 +46:02:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:32.17 +47:44:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:32.39 +47:13:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:32.66 +47:50:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:33.41 +46:11:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:33.44 +47:18:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:33.79 +46:02:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:34.86 +43:35:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:35.28 +47:24:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:36.54 +47:07:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:36.59 +46:43:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:36.59 +47:34:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:37.03 +43:27:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:38.07 +43:06:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:38.41 +46:18:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:38.56 +47:22:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:39.88 +45:56:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:39.93 +43:55:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:40.40 +46:34:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:40.49 +46:31:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:42.57 +42:56:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:42.60 +46:05:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:42.63 +47:57:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:42.77 +47:15:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:43.22 +46:17:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:44.25 +45:45:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:44.34 +47:03:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.06 +45:56:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.40 +46:21:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.71 +47:20:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.74 +46:54:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.91 +43:27:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.94 +47:23:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.98 +44:02:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:46.19 +46:09:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:46.38 +43:42:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:46.70 +45:54:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:46.97 +47:25:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:47.69 +42:44:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:48.44 +46:02:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:48.86 +47:27:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:50.41 +47:55:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:50.57 +46:14:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:51.20 +47:22:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:51.62 +47:43:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:51.97 +46:37:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:53.32 +42:46:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:53.80 +47:35:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:54.64 +42:42:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:54.84 +46:14:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:55.27 +47:03:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:55.93 +46:00:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:56.03 +46:21:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:56.64 +46:52:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:56.76 +46:26:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:57.15 +47:04:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:58.11 +46:44:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:58.90 +47:51:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:59.88 +47:36:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:59.98 +47:07:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:00.34 +44:02:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:03.42 +46:24:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:03.65 +47:07:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:04.36 +43:52:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:04.66 +47:33:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:04.87 +46:52:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:04.89 +47:19:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:05.80 +43:40:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:05.91 +46:40:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:07.28 +46:39:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:07.48 +43:22:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:09.12 +42:18:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:09.50 +47:08:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:09.60 +46:09:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:10.08 +46:24:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:10.79 +47:26:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:12.13 +47:16:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:13.39 +47:06:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:14.83 +47:06:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:14.94 +46:25:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:15.01 +47:25:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:15.11 +47:36:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:17.05 +45:55:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:18.90 +47:12:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:19.26 +47:41:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:19.73 +42:51:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:22.01 +47:34:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:22.22 +42:50:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:22.54 +47:12:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:23.13 +47:46:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:23.53 +42:21:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:25.44 +47:00:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:27.46 +47:00:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:27.96 +46:42:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:29.02 +46:43:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:29.34 +47:42:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:30.15 +47:38:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:33.13 +41:55:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:33.31 +46:38:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:34.58 +47:05:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:34.91 +46:47:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:36.53 +46:30:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:36.73 +47:02:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:38.80 +47:33:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:41.13 +47:17:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:43.22 +46:59:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:45.20 +47:29:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:45.62 +46:26:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:45.85 +44:01:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:46.06 +47:00:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:46.16 +47:42:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:47.34 +43:03:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:48.65 +47:30:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:49.04 +47:01:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:50.98 +47:39:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:52.14 +47:37:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:52.24 +46:46:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:52.62 +47:33:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:53.33 +47:14:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:53.71 +43:52:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:56.12 +47:08:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:56.66 +46:45:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:57.53 +47:28:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:57.56 +47:27:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:57.65 +43:48:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:58.76 +47:52:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:08.72 +47:36:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:11.28 +44:29:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:11.47 +47:45:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:12.16 +43:19:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:12.89 +47:51:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:13.44 +47:09:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:14.96 +47:40:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:15.41 +47:54:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:16.95 +47:18:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:20.15 +47:52:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:21.25 +46:58:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:25.10 +46:44:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:25.89 +47:38:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:30.15 +46:45:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:33.87 +47:53:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:39.39 +42:08:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:40.21 +47:51:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:42.43 +47:50:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:43.22 +47:52:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:43.86 +47:57:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:44.81 +47:54:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:44.95 +47:40:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:46.68 +47:28:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:50.43 +47:55:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:52.08 +42:49:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:53.32 +43:09:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:02.74 +47:01:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:04.48 +47:50:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:18.36 +47:48:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:25.45 +47:57:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:25.79 +44:12:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:43.18 +47:51:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:49.68 +44:12:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:06:52.19 +43:27:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:45.05 +47:24:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:08.42 +48:51:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:14.90 +48:18:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:33.02 +48:40:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:53.92 +47:22:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:30.25 +45:06:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:38.64 +45:34:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:17.87 +43:02:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:14.43 +43:52:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:16.74 +42:26:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:28.77 +42:04:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:11.37 +42:48:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:48.36 +42:11:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:51.65 +43:04:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:57.21 +42:29:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:58.96 +42:53:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:07.22 +42:35:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:11.13 +42:55:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:16.45 +42:46:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:17.27 +43:12:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:28.34 +42:57:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:38.76 +42:32:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:42.49 +42:28:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:42.58 +43:28:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:55.36 +42:45:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:56.50 +43:29:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:07.74 +43:21:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:13.13 +43:16:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:18.50 +43:17:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:28.69 +42:50:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:28.79 +42:49:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:35.88 +43:06:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:38.34 +43:18:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:55.45 +43:13:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:01.85 +43:44:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:13.11 +42:38:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:14.65 +43:36:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:18.09 +42:50:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:18.98 +43:57:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:21.11 +43:32:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:28.59 +42:48:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:31.19 +43:06:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:35.41 +43:40:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:38.89 +43:37:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:55.89 +44:15:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:59.41 +43:25:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:15.59 +43:58:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:16.56 +43:16:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:27.49 +43:26:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:30.99 +42:43:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.00 +43:37:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.68 +43:49:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:41.65 +43:53:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:41.77 +43:56:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:45.84 +43:28:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:48.67 +43:42:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:54.86 +43:34:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:01.30 +44:39:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:07.04 +43:56:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:19.54 +43:43:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:20.75 +44:00:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:21.29 +43:25:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:23.45 +43:35:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:29.24 +44:32:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:37.38 +44:29:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:40.24 +44:01:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:47.46 +43:43:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:00.54 +44:26:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:01.76 +43:46:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:10.62 +43:40:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:13.65 +43:43:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:20.28 +44:04:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:26.80 +43:50:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:31.69 +43:57:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:34.48 +44:10:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:41.09 +43:22:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:46.23 +44:12:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:50.91 +43:45:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:57.85 +44:28:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:08.06 +44:35:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:12.83 +44:01:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:17.98 +44:02:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:27.62 +44:51:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:36.69 +44:56:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:59.36 +45:03:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:37.88 +43:08:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:49.64 +46:37:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:55.68 +45:48:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:44.28 +46:55:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:56.55 +43:22:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:51.26 +49:07:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:55.12 +48:46:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:19.91 +48:50:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:50.22 +48:57:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:01.64 +49:22:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:11.03 +49:35:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:29.70 +49:22:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:52.94 +49:38:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:04.37 +49:35:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:06.72 +49:32:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:11.13 +49:35:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:21.99 +49:22:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:00:00.92 +47:54:55.5 -- not a known variable star
21:00:06.14 +47:56:10.5 -- a known variable star
21:00:06.21 +47:39:07.4 -- not a known variable star
21:00:07.72 +47:50:00.1 -- a known variable star
21:00:08.77 +47:34:15.5 -- not a known variable star
21:00:10.42 +47:56:08.5 -- a known variable star
21:00:11.76 +47:53:24.2 -- not a known variable star
21:00:12.04 +47:54:15.9 -- not a known variable star
21:00:12.39 +47:32:58.4 -- not a known variable star
21:00:14.05 +47:53:01.5 -- a known variable star
21:00:15.24 +47:16:52.5 -- not a known variable star
21:00:16.39 +47:15:21.2 -- not a known variable star
21:00:16.81 +47:41:00.9 -- not a known variable star
21:00:16.88 +47:12:34.7 -- not a known variable star
21:00:16.89 +47:16:05.1 -- not a known variable star
21:00:17.91 +47:39:14.5 -- not a known variable star
21:00:18.71 +47:17:58.3 -- not a known variable star
21:00:19.63 +47:39:08.7 -- not a known variable star
21:00:20.31 +47:31:07.4 -- not a known variable star
21:00:20.53 +47:35:01.6 -- not a known variable star
21:00:20.56 +47:32:40.1 -- not a known variable star
21:00:20.58 +47:45:34.2 -- not a known variable star
21:00:21.45 +47:50:50.7 -- a known variable star
21:00:21.50 +47:29:48.5 -- not a known variable star
21:00:22.20 +46:58:48.4 -- not a known variable star
21:00:23.24 +46:57:54.6 -- not a known variable star
21:00:24.33 +47:43:19.3 -- not a known variable star
21:00:24.54 +47:27:40.6 -- not a known variable star
21:00:24.57 +47:20:44.2 -- not a known variable star
21:00:24.64 +47:32:02.6 -- a known variable star
21:00:24.71 +46:51:21.6 -- not a known variable star
21:00:24.76 +47:29:12.8 -- not a known variable star
21:00:24.83 +47:45:31.2 -- not a known variable star
21:00:25.41 +47:47:45.1 -- not a known variable star
21:00:26.30 +47:45:58.8 -- not a known variable star
21:00:26.69 +47:04:58.5 -- a known variable star
21:00:26.73 +47:46:46.9 -- not a known variable star
21:00:26.99 +47:16:52.7 -- a known variable star
21:00:27.86 +47:11:35.8 -- not a known variable star
21:00:28.29 +46:48:39.2 -- not a known variable star
21:00:28.66 +46:35:37.0 -- not a known variable star
21:00:29.52 +47:56:56.5 -- a known variable star
21:00:29.82 +47:52:19.3 -- not a known variable star
21:00:30.78 +46:33:01.4 -- a known variable star
21:00:31.27 +46:49:47.5 -- not a known variable star
21:00:31.68 +47:20:36.3 -- not a known variable star
21:00:32.39 +47:01:19.4 -- not a known variable star
21:00:33.37 +47:29:25.6 -- not a known variable star
21:00:33.77 +47:46:33.7 -- not a known variable star
21:00:33.85 +46:28:25.5 -- a known variable star
21:00:34.61 +46:56:48.7 -- not a known variable star
21:00:34.83 +47:23:01.6 -- a known variable star
21:00:35.25 +47:07:08.6 -- not a known variable star
21:00:35.49 +47:06:30.4 -- not a known variable star
21:00:35.54 +47:02:37.3 -- not a known variable star
21:00:36.25 +46:12:48.1 -- not a known variable star
21:00:36.27 +46:25:02.5 -- not a known variable star
21:00:36.46 +47:54:44.4 -- not a known variable star
21:00:36.95 +47:12:33.2 -- a known variable star
21:00:37.18 +47:50:17.6 -- not a known variable star
21:00:39.36 +47:14:04.7 -- not a known variable star
21:00:39.39 +47:48:27.1 -- not a known variable star
21:00:39.55 +47:49:42.1 -- not a known variable star
21:00:39.72 +47:21:26.7 -- not a known variable star
21:00:40.04 +47:48:49.8 -- not a known variable star
21:00:41.62 +47:23:33.7 -- not a known variable star
21:00:42.01 +46:29:12.5 -- not a known variable star
21:00:43.49 +47:43:24.8 -- not a known variable star
21:00:43.92 +47:19:26.9 -- not a known variable star
21:00:44.06 +47:50:17.9 -- not a known variable star
21:00:44.11 +46:15:56.8 -- not a known variable star
21:00:44.45 +46:06:59.7 -- not a known variable star
21:00:45.23 +46:59:42.9 -- not a known variable star
21:00:45.51 +47:30:06.6 -- a known variable star
21:00:45.63 +46:17:54.1 -- not a known variable star
21:00:46.35 +47:54:14.8 -- not a known variable star
21:00:46.59 +47:34:58.1 -- not a known variable star
21:00:46.75 +45:41:15.1 -- not a known variable star
21:00:47.85 +47:07:24.2 -- not a known variable star
21:00:48.71 +47:19:28.6 -- a known variable star
21:00:48.90 +46:26:08.0 -- not a known variable star
21:00:48.99 +46:02:47.9 -- not a known variable star
21:00:48.99 +46:29:42.1 -- not a known variable star
21:00:49.09 +46:58:36.9 -- not a known variable star
21:00:49.12 +46:27:02.3 -- a known variable star
21:00:49.27 +47:13:06.5 -- not a known variable star
21:00:49.41 +47:42:57.7 -- not a known variable star
21:00:49.47 +47:13:47.2 -- not a known variable star
21:00:50.61 +47:55:23.3 -- not a known variable star
21:00:51.08 +46:38:28.1 -- not a known variable star
21:00:51.09 +47:16:30.5 -- a known variable star
21:00:51.77 +46:57:05.1 -- not a known variable star
21:00:51.95 +47:44:30.1 -- not a known variable star
21:00:52.11 +46:49:27.3 -- not a known variable star
21:00:52.61 +47:33:02.8 -- not a known variable star
21:00:52.66 +47:40:07.2 -- not a known variable star
21:00:53.18 +46:05:45.8 -- a known variable star
21:00:54.20 +47:54:28.5 -- not a known variable star
21:00:55.88 +46:42:56.8 -- not a known variable star
21:00:55.95 +47:31:10.3 -- not a known variable star
21:00:56.50 +46:41:10.3 -- not a known variable star
21:00:56.58 +45:47:09.1 -- a known variable star
21:00:56.64 +47:45:39.5 -- not a known variable star
21:00:57.59 +46:25:05.4 -- not a known variable star
21:00:58.41 +47:25:47.5 -- not a known variable star
21:00:58.49 +47:00:10.6 -- not a known variable star
21:00:58.52 +46:58:58.6 -- not a known variable star
21:00:59.22 +47:53:10.6 -- not a known variable star
21:01:00.05 +47:41:38.6 -- not a known variable star
21:01:01.04 +47:07:14.8 -- not a known variable star
21:01:01.14 +47:34:18.5 -- a known variable star
21:01:01.46 +47:51:41.2 -- not a known variable star
21:01:01.67 +46:30:17.8 -- not a known variable star
21:01:01.71 +45:55:07.6 -- a known variable star
21:01:01.95 +47:48:45.1 -- not a known variable star
21:01:02.34 +45:40:24.0 -- not a known variable star
21:01:02.48 +45:57:30.3 -- not a known variable star
21:01:03.33 +47:06:17.9 -- not a known variable star
21:01:03.89 +47:20:01.0 -- not a known variable star
21:01:04.14 +47:53:15.6 -- not a known variable star
21:01:04.52 +45:39:42.1 -- not a known variable star
21:01:04.56 +46:16:22.9 -- a known variable star
21:01:04.72 +47:48:55.0 -- a known variable star
21:01:05.42 +46:49:26.4 -- not a known variable star
21:01:05.78 +47:40:22.0 -- not a known variable star
21:01:06.42 +47:49:44.7 -- not a known variable star
21:01:06.83 +45:55:39.0 -- not a known variable star
21:01:07.13 +46:33:32.6 -- a known variable star
21:01:07.55 +47:42:54.5 -- a known variable star
21:01:07.73 +46:02:12.6 -- not a known variable star
21:01:07.74 +47:34:38.7 -- not a known variable star
21:01:07.81 +47:25:27.1 -- not a known variable star
21:01:08.44 +45:39:36.1 -- not a known variable star
21:01:08.50 +47:39:27.5 -- not a known variable star
21:01:08.77 +47:09:53.6 -- not a known variable star
21:01:09.22 +46:18:42.9 -- not a known variable star
21:01:09.91 +47:44:33.2 -- not a known variable star
21:01:10.16 +46:21:53.8 -- not a known variable star
21:01:10.40 +47:31:34.0 -- a known variable star
21:01:10.79 +46:46:08.5 -- not a known variable star
21:01:11.17 +46:11:52.3 -- not a known variable star
21:01:11.17 +47:15:47.2 -- not a known variable star
21:01:11.25 +47:34:36.1 -- not a known variable star
21:01:11.38 +47:47:18.4 -- not a known variable star
21:01:11.44 +46:27:37.4 -- a known variable star
21:01:12.60 +46:58:06.7 -- not a known variable star
21:01:12.66 +47:53:16.1 -- not a known variable star
21:01:12.75 +45:54:49.6 -- not a known variable star
21:01:13.23 +46:58:38.3 -- not a known variable star
21:01:14.98 +47:20:40.5 -- not a known variable star
21:01:15.69 +47:12:56.9 -- a known variable star
21:01:15.87 +47:22:29.0 -- a known variable star
21:01:15.94 +47:57:35.1 -- not a known variable star
21:01:16.29 +47:39:54.8 -- not a known variable star
21:01:17.60 +46:44:42.6 -- not a known variable star
21:01:17.70 +46:39:32.3 -- not a known variable star
21:01:17.73 +46:40:29.7 -- not a known variable star
21:01:17.95 +46:45:47.3 -- not a known variable star
21:01:18.32 +46:38:44.2 -- not a known variable star
21:01:18.55 +46:41:12.8 -- a known variable star
21:01:19.24 +46:32:51.4 -- a known variable star
21:01:19.42 +46:58:50.7 -- not a known variable star
21:01:19.61 +47:16:27.8 -- not a known variable star
21:01:19.74 +46:38:16.3 -- not a known variable star
21:01:20.96 +47:10:44.2 -- not a known variable star
21:01:21.15 +47:05:57.4 -- a known variable star
21:01:21.65 +47:02:22.6 -- not a known variable star
21:01:21.88 +45:36:50.8 -- a known variable star
21:01:22.16 +46:19:21.6 -- a known variable star
21:01:22.53 +46:40:19.8 -- not a known variable star
21:01:22.56 +47:30:32.2 -- not a known variable star
21:01:23.37 +47:05:14.4 -- not a known variable star
21:01:23.78 +47:15:38.4 -- not a known variable star
21:01:24.12 +47:53:37.8 -- not a known variable star
21:01:24.29 +47:48:25.7 -- not a known variable star
21:01:24.45 +46:22:15.9 -- not a known variable star
21:01:25.22 +46:51:10.3 -- not a known variable star
21:01:26.14 +45:46:14.3 -- a known variable star
21:01:26.19 +46:58:32.2 -- not a known variable star
21:01:27.53 +47:21:36.3 -- not a known variable star
21:01:27.70 +47:17:20.1 -- not a known variable star
21:01:27.88 +46:42:29.0 -- not a known variable star
21:01:29.04 +46:11:49.8 -- a known variable star
21:01:29.17 +46:29:55.8 -- not a known variable star
21:01:29.37 +46:29:00.9 -- a known variable star
21:01:30.61 +46:16:02.9 -- not a known variable star
21:01:31.06 +46:50:45.4 -- not a known variable star
21:01:32.15 +46:02:08.2 -- not a known variable star
21:01:32.17 +47:44:22.2 -- not a known variable star
21:01:32.39 +47:13:17.3 -- a known variable star
21:01:32.66 +47:50:45.8 -- not a known variable star
21:01:33.41 +46:11:37.4 -- a known variable star
21:01:33.44 +47:18:42.9 -- a known variable star
21:01:33.79 +46:02:45.1 -- a known variable star
21:01:34.86 +43:35:54.5 -- not a known variable star
21:01:35.28 +47:24:12.4 -- not a known variable star
21:01:36.54 +47:07:10.9 -- not a known variable star
21:01:36.59 +46:43:18.2 -- not a known variable star
21:01:36.59 +47:34:59.8 -- not a known variable star
21:01:37.03 +43:27:40.2 -- not a known variable star
21:01:38.07 +43:06:18.6 -- not a known variable star
21:01:38.41 +46:18:07.8 -- a known variable star
21:01:38.56 +47:22:15.5 -- not a known variable star
21:01:39.88 +45:56:16.0 -- not a known variable star
21:01:39.93 +43:55:06.2 -- not a known variable star
21:01:40.40 +46:34:08.0 -- not a known variable star
21:01:40.49 +46:31:53.7 -- a known variable star
21:01:42.57 +42:56:49.8 -- not a known variable star
21:01:42.60 +46:05:33.5 -- a known variable star
21:01:42.63 +47:57:46.5 -- not a known variable star
21:01:42.77 +47:15:05.6 -- not a known variable star
21:01:43.22 +46:17:05.5 -- not a known variable star
21:01:44.25 +45:45:58.0 -- not a known variable star
21:01:44.34 +47:03:38.9 -- not a known variable star
21:01:45.06 +45:56:35.4 -- a known variable star
21:01:45.40 +46:21:17.7 -- a known variable star
21:01:45.71 +47:20:23.6 -- not a known variable star
21:01:45.74 +46:54:02.4 -- not a known variable star
21:01:45.91 +43:27:30.6 -- not a known variable star
21:01:45.94 +47:23:15.0 -- not a known variable star
21:01:45.98 +44:02:42.1 -- not a known variable star
21:01:46.19 +46:09:51.8 -- not a known variable star
21:01:46.38 +43:42:50.7 -- not a known variable star
21:01:46.70 +45:54:21.4 -- a known variable star
21:01:46.97 +47:25:14.5 -- not a known variable star
21:01:47.69 +42:44:55.1 -- not a known variable star
21:01:48.44 +46:02:22.3 -- a known variable star
21:01:48.86 +47:27:56.4 -- a known variable star
21:01:50.41 +47:55:02.9 -- not a known variable star
21:01:50.57 +46:14:12.1 -- a known variable star
21:01:51.20 +47:22:01.5 -- not a known variable star
21:01:51.62 +47:43:23.7 -- not a known variable star
21:01:51.97 +46:37:43.6 -- not a known variable star
21:01:53.32 +42:46:25.5 -- not a known variable star
21:01:53.80 +47:35:41.1 -- a known variable star
21:01:54.64 +42:42:36.2 -- not a known variable star
21:01:54.84 +46:14:13.6 -- not a known variable star
21:01:55.27 +47:03:18.7 -- a known variable star
21:01:55.93 +46:00:20.1 -- not a known variable star
21:01:56.03 +46:21:42.6 -- a known variable star
21:01:56.64 +46:52:04.3 -- not a known variable star
21:01:56.76 +46:26:30.0 -- not a known variable star
21:01:57.15 +47:04:09.8 -- not a known variable star
21:01:58.11 +46:44:17.8 -- a known variable star
21:01:58.90 +47:51:02.7 -- not a known variable star
21:01:59.88 +47:36:05.9 -- not a known variable star
21:01:59.98 +47:07:19.4 -- not a known variable star
21:02:00.34 +44:02:06.9 -- not a known variable star
21:02:03.42 +46:24:30.7 -- a known variable star
21:02:03.65 +47:07:10.0 -- not a known variable star
21:02:04.36 +43:52:52.1 -- not a known variable star
21:02:04.66 +47:33:53.5 -- not a known variable star
21:02:04.87 +46:52:03.5 -- not a known variable star
21:02:04.89 +47:19:57.6 -- not a known variable star
21:02:05.80 +43:40:49.4 -- not a known variable star
21:02:05.91 +46:40:05.4 -- not a known variable star
21:02:07.28 +46:39:22.5 -- not a known variable star
21:02:07.48 +43:22:28.0 -- not a known variable star
21:02:09.12 +42:18:06.5 -- not a known variable star
21:02:09.50 +47:08:39.4 -- not a known variable star
21:02:09.60 +46:09:28.1 -- not a known variable star
21:02:10.08 +46:24:26.4 -- a known variable star
21:02:10.79 +47:26:29.8 -- not a known variable star
21:02:12.13 +47:16:49.6 -- not a known variable star
21:02:13.39 +47:06:48.4 -- a known variable star
21:02:14.83 +47:06:29.7 -- a known variable star
21:02:14.94 +46:25:35.7 -- not a known variable star
21:02:15.01 +47:25:04.4 -- a known variable star
21:02:15.11 +47:36:31.5 -- not a known variable star
21:02:17.05 +45:55:58.5 -- not a known variable star
21:02:18.90 +47:12:14.3 -- not a known variable star
21:02:19.26 +47:41:50.1 -- not a known variable star
21:02:19.73 +42:51:14.0 -- not a known variable star
21:02:22.01 +47:34:49.1 -- not a known variable star
21:02:22.22 +42:50:31.9 -- not a known variable star
21:02:22.54 +47:12:04.9 -- not a known variable star
21:02:23.13 +47:46:41.1 -- not a known variable star
21:02:23.53 +42:21:57.0 -- not a known variable star
21:02:25.44 +47:00:50.4 -- not a known variable star
21:02:27.46 +47:00:00.9 -- not a known variable star
21:02:27.96 +46:42:00.0 -- a known variable star
21:02:29.02 +46:43:18.5 -- not a known variable star
21:02:29.34 +47:42:30.7 -- not a known variable star
21:02:30.15 +47:38:53.2 -- not a known variable star
21:02:33.13 +41:55:25.8 -- not a known variable star
21:02:33.31 +46:38:50.7 -- not a known variable star
21:02:34.58 +47:05:41.7 -- a known variable star
21:02:34.91 +46:47:04.7 -- not a known variable star
21:02:36.53 +46:30:50.2 -- a known variable star
21:02:36.73 +47:02:34.5 -- not a known variable star
21:02:38.80 +47:33:01.7 -- not a known variable star
21:02:41.13 +47:17:01.0 -- not a known variable star
21:02:43.22 +46:59:46.5 -- not a known variable star
21:02:45.20 +47:29:25.4 -- not a known variable star
21:02:45.62 +46:26:49.9 -- a known variable star
21:02:45.85 +44:01:19.2 -- not a known variable star
21:02:46.06 +47:00:34.9 -- not a known variable star
21:02:46.16 +47:42:36.8 -- not a known variable star
21:02:47.34 +43:03:31.5 -- not a known variable star
21:02:48.65 +47:30:14.0 -- not a known variable star
21:02:49.04 +47:01:18.2 -- not a known variable star
21:02:50.98 +47:39:38.5 -- not a known variable star
21:02:52.14 +47:37:54.6 -- not a known variable star
21:02:52.24 +46:46:50.6 -- a known variable star
21:02:52.62 +47:33:34.2 -- not a known variable star
21:02:53.33 +47:14:25.7 -- not a known variable star
21:02:53.71 +43:52:57.2 -- not a known variable star
21:02:56.12 +47:08:25.4 -- not a known variable star
21:02:56.66 +46:45:03.2 -- not a known variable star
21:02:57.53 +47:28:31.1 -- not a known variable star
21:02:57.56 +47:27:45.7 -- not a known variable star
21:02:57.65 +43:48:19.2 -- not a known variable star
21:02:58.76 +47:52:40.4 -- not a known variable star
21:03:08.72 +47:36:12.4 -- not a known variable star
21:03:11.28 +44:29:58.6 -- not a known variable star
21:03:11.47 +47:45:34.0 -- not a known variable star
21:03:12.16 +43:19:50.4 -- not a known variable star
21:03:12.89 +47:51:12.9 -- not a known variable star
21:03:13.44 +47:09:13.3 -- not a known variable star
21:03:14.96 +47:40:60.0 -- a known variable star
21:03:15.41 +47:54:39.8 -- not a known variable star
21:03:16.95 +47:18:56.9 -- not a known variable star
21:03:20.15 +47:52:05.2 -- not a known variable star
21:03:21.25 +46:58:15.0 -- not a known variable star
21:03:25.10 +46:44:04.1 -- not a known variable star
21:03:25.89 +47:38:60.0 -- not a known variable star
21:03:30.15 +46:45:00.1 -- not a known variable star
21:03:33.87 +47:53:01.8 -- a known variable star
21:03:39.39 +42:08:18.3 -- a known variable star
21:03:40.21 +47:51:05.9 -- a known variable star
21:03:42.43 +47:50:10.8 -- a known variable star
21:03:43.22 +47:52:40.9 -- not a known variable star
21:03:43.86 +47:57:01.8 -- not a known variable star
21:03:44.81 +47:54:42.4 -- not a known variable star
21:03:44.95 +47:40:16.8 -- not a known variable star
21:03:46.68 +47:28:32.4 -- a known variable star
21:03:50.43 +47:55:38.6 -- not a known variable star
21:03:52.08 +42:49:39.7 -- not a known variable star
21:03:53.32 +43:09:58.8 -- not a known variable star
21:04:02.74 +47:01:40.7 -- a known variable star
21:04:04.48 +47:50:17.6 -- not a known variable star
21:04:18.36 +47:48:57.0 -- not a known variable star
21:04:25.45 +47:57:28.0 -- a known variable star
21:04:25.79 +44:12:40.7 -- not a known variable star
21:04:43.18 +47:51:03.8 -- not a known variable star
21:04:49.68 +44:12:50.6 -- not a known variable star
21:06:52.19 +43:27:55.1 -- not a known variable star
21:08:45.05 +47:24:08.6 -- a known variable star
21:10:08.42 +48:51:33.8 -- a known variable star
21:10:14.90 +48:18:57.5 -- a known variable star
21:10:33.02 +48:40:56.5 -- not a known variable star
21:10:53.92 +47:22:42.5 -- not a known variable star
21:11:30.25 +45:06:16.2 -- a known variable star
21:35:38.64 +45:34:17.4 -- a known variable star
21:36:17.87 +43:02:43.0 -- a known variable star
21:37:14.43 +43:52:38.5 -- a known variable star
21:39:16.74 +42:26:30.7 -- a known variable star
21:39:28.77 +42:04:37.6 -- a known variable star
21:40:11.37 +42:48:51.6 -- not a known variable star
21:40:48.36 +42:11:06.3 -- a known variable star
21:40:51.65 +43:04:31.4 -- not a known variable star
21:40:57.21 +42:29:09.1 -- not a known variable star
21:40:58.96 +42:53:16.0 -- not a known variable star
21:41:07.22 +42:35:09.6 -- not a known variable star
21:41:11.13 +42:55:31.4 -- a known variable star
21:41:16.45 +42:46:22.6 -- not a known variable star
21:41:17.27 +43:12:56.5 -- not a known variable star
21:41:28.34 +42:57:28.9 -- not a known variable star
21:41:38.76 +42:32:27.2 -- not a known variable star
21:41:42.49 +42:28:26.3 -- not a known variable star
21:41:42.58 +43:28:15.8 -- not a known variable star
21:41:55.36 +42:45:07.1 -- a known variable star
21:41:56.50 +43:29:18.8 -- a known variable star
21:42:07.74 +43:21:56.0 -- not a known variable star
21:42:13.13 +43:16:50.4 -- not a known variable star
21:42:18.50 +43:17:39.2 -- not a known variable star
21:42:28.69 +42:50:57.8 -- a known variable star
21:42:28.79 +42:49:49.7 -- not a known variable star
21:42:35.88 +43:06:07.4 -- not a known variable star
21:42:38.34 +43:18:23.7 -- a known variable star
21:42:55.45 +43:13:24.3 -- not a known variable star
21:43:01.85 +43:44:28.6 -- not a known variable star
21:43:13.11 +42:38:46.9 -- not a known variable star
21:43:14.65 +43:36:25.3 -- a known variable star
21:43:18.09 +42:50:50.1 -- not a known variable star
21:43:18.98 +43:57:57.5 -- a known variable star
21:43:21.11 +43:32:30.7 -- not a known variable star
21:43:28.59 +42:48:18.0 -- a known variable star
21:43:31.19 +43:06:41.4 -- a known variable star
21:43:35.41 +43:40:39.7 -- not a known variable star
21:43:38.89 +43:37:42.6 -- not a known variable star
21:43:55.89 +44:15:44.6 -- not a known variable star
21:43:59.41 +43:25:19.2 -- not a known variable star
21:44:15.59 +43:58:12.3 -- not a known variable star
21:44:16.56 +43:16:44.0 -- not a known variable star
21:44:27.49 +43:26:11.4 -- not a known variable star
21:44:30.99 +42:43:17.8 -- not a known variable star
21:44:37.00 +43:37:40.5 -- not a known variable star
21:44:37.68 +43:49:23.1 -- not a known variable star
21:44:41.65 +43:53:38.5 -- not a known variable star
21:44:41.77 +43:56:20.6 -- a known variable star
21:44:45.84 +43:28:19.3 -- a known variable star
21:44:48.67 +43:42:11.4 -- not a known variable star
21:44:54.86 +43:34:13.9 -- not a known variable star
21:45:01.30 +44:39:16.3 -- a known variable star
21:45:07.04 +43:56:01.9 -- not a known variable star
21:45:19.54 +43:43:55.8 -- not a known variable star
21:45:20.75 +44:00:03.1 -- not a known variable star
21:45:21.29 +43:25:05.6 -- not a known variable star
21:45:23.45 +43:35:34.9 -- not a known variable star
21:45:29.24 +44:32:48.5 -- a known variable star
21:45:37.38 +44:29:47.5 -- a known variable star
21:45:40.24 +44:01:21.8 -- not a known variable star
21:45:47.46 +43:43:38.4 -- not a known variable star
21:46:00.54 +44:26:43.7 -- not a known variable star
21:46:01.76 +43:46:35.9 -- not a known variable star
21:46:10.62 +43:40:56.1 -- not a known variable star
21:46:13.65 +43:43:19.4 -- not a known variable star
21:46:20.28 +44:04:46.1 -- not a known variable star
21:46:26.80 +43:50:35.2 -- not a known variable star
21:46:31.69 +43:57:33.9 -- a known variable star
21:46:34.48 +44:10:35.1 -- a known variable star
21:46:41.09 +43:22:37.1 -- not a known variable star
21:46:46.23 +44:12:42.3 -- not a known variable star
21:46:50.91 +43:45:47.6 -- not a known variable star
21:46:57.85 +44:28:25.6 -- not a known variable star
21:47:08.06 +44:35:10.4 -- not a known variable star
21:47:12.83 +44:01:35.8 -- not a known variable star
21:47:17.98 +44:02:39.3 -- not a known variable star
21:48:27.62 +44:51:17.4 -- not a known variable star
21:48:36.69 +44:56:50.0 -- a known variable star
21:49:59.36 +45:03:44.4 -- a known variable star
21:50:37.88 +43:08:50.2 -- a known variable star
21:52:49.64 +46:37:11.7 -- a known variable star
21:56:55.68 +45:48:32.0 -- a known variable star
21:58:44.28 +46:55:38.0 -- not a known variable star
21:58:56.55 +43:22:56.1 -- a known variable star
22:06:51.26 +49:07:03.3 -- a known variable star
22:06:55.12 +48:46:16.3 -- a known variable star
22:07:19.91 +48:50:45.8 -- a known variable star
22:07:50.22 +48:57:43.0 -- not a known variable star
22:09:01.64 +49:22:14.8 -- not a known variable star
22:09:11.03 +49:35:48.1 -- not a known variable star
22:09:29.70 +49:22:38.6 -- not a known variable star
22:10:52.94 +49:38:37.7 -- not a known variable star
22:11:04.37 +49:35:08.6 -- not a known variable star
22:12:06.72 +49:32:35.2 -- a known variable star
22:12:11.13 +49:35:54.6 -- not a known variable star
22:12:21.99 +49:22:24.0 -- not a known variable star
Found 341 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
449 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 449 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461124.95519410 -observatory 500
22:42:58.23 -08:13:46.3 Mercury (0.7mag)
01:26:55.35 +08:21:52.6 Venus (-3.9mag)
23:16:07.82 -05:52:14.9 Mars (1.2mag)
07:05:30.58 +22:57:03.7 Jupiter (-2.3mag)
00:19:23.44 -00:13:01.1 Saturn (0.9mag)
03:43:38.18 +19:34:13.2 Uranus (5.8mag)
00:07:54.59 -00:34:02.2 Neptune (7.8mag)
20:32:23.28 -22:53:15.4 Pluto (14.5mag)
05:59:20.22 +28:18:15.0 Moon (-10.2mag)
-rw-r--r-- 1 apache apache 362 Mar 25 05:58 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461124.95519410:
07:05:22.06 +22:57:20.1 Io (5.6mag)
07:05:28.26 +22:57:11.3 Europa (5.8mag)
07:05:49.78 +22:56:23.8 Ganymede (5.2mag)
07:05:20.23 +22:57:33.0 Callisto (6.4mag)
07:09:29.77 +22:56:05.2 Himalia (15.2mag)
07:05:31.01 +22:57:00.0 Thebe (16.1mag)
07:09:10.41 +23:21:13.8 Elara (17.2mag)
07:02:56.11 +23:48:23.0 Pasiphae (17.2mag)
07:14:14.26 +22:52:17.8 Carme (18.3mag)
00:19:34.01 -00:13:07.8 Titan (8.8mag)
00:19:27.66 -00:13:00.4 Rhea (10.1mag)
00:19:47.91 -00:10:49.2 Iapetus (11.5mag)
00:19:32.30 -00:12:45.0 Hyperion (14.8mag)
00:21:15.12 -00:02:07.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 25 05:58 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461124.95519410:
13:25:40.50 +04:01:12.6 JWST
19:33:42.07 +07:49:29.2 Chandra
09:09:37.10 -49:30:27.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 25 05:58 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461124.95519410 -observatory 500
18:39:02.92 -27:39:43.7 14.0mag P/2010 H2 (Vales)
04:53:20.34 -70:46:53.5 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:04.18 +31:19:01.9 17.1mag C/2017 K2 (PANSTARRS)
17:30:15.80 +07:56:34.9 17.6mag C/2021 G2 (ATLAS)
23:03:15.80 +28:31:52.9 16.9mag C/2022 E2 (ATLAS)
04:05:09.49 +25:25:25.1 15.8mag C/2022 N2 (PANSTARRS)
09:01:33.89 +31:36:41.6 16.0mag C/2022 QE78 (ATLAS)
08:29:53.27 -02:37:33.3 17.2mag C/2022 R6 (PANSTARRS)
18:56:30.38 +16:40:32.0 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:49.27 -11:48:07.3 17.6mag P/2023 B1 (PANSTARRS)
09:20:56.04 -15:32:31.1 17.4mag C/2023 F3 (ATLAS)
21:28:10.91 +61:51:17.4 17.4mag C/2023 H5 (Lemmon)
19:31:53.05 -03:32:09.0 14.4mag C/2023 R1 (PANSTARRS)
21:39:43.25 +83:16:56.5 17.7mag C/2023 X2 (Lemmon)
06:14:16.43 +63:43:33.0 16.9mag C/2024 A1 (ATLAS)
04:20:03.41 +08:17:04.9 9.5mag C/2024 E1 (Wierzchos)
11:18:59.73 +03:36:18.1 18.0mag C/2024 G2 (ATLAS)
16:30:37.06 +02:52:14.3 17.5mag C/2024 G6 (ATLAS)
20:12:20.81 +09:47:52.5 14.8mag C/2024 J3 (ATLAS)
03:08:08.38 -25:52:49.1 16.4mag C/2024 T5 (ATLAS)
05:00:17.20 +51:13:00.1 17.6mag C/2025 J1 (Borisov)
15:00:53.63 +23:26:30.3 14.5mag C/2025 L1 (ATLAS)
02:54:11.82 -23:09:14.6 17.7mag C/2025 Q3 (ATLAS)
22:36:11.65 +19:19:00.9 11.9mag C/2025 R3 (PANSTARRS)
13:03:19.66 +01:36:35.3 17.6mag C/2025 Y1 (ATLAS)
01:57:30.14 -03:33:13.9 13.0mag C/2026 A1 (MAPS)
22:53:43.11 +32:19:53.4 13.9mag C/2026 B2 (Sun-Gao)
18:00:47.71 -10:42:02.4 13.1mag 10P/Tempel
15:24:09.12 +04:53:56.0 12.1mag 24P/Schaumasse
11:10:09.52 -02:18:30.9 15.6mag 29P/Schwassmann-Wachmann
17:47:59.60 -10:28:18.8 17.4mag 40P/Vaisala
10:42:57.95 -06:06:31.9 16.5mag 43P/Wolf-Harrington
01:15:40.54 +13:43:20.1 17.0mag 47P/Ashbrook-Jackson
06:34:48.27 +41:27:47.8 17.1mag 63P/Wild
23:00:24.42 -14:09:29.8 15.7mag 65P/Gunn
03:08:53.57 +13:09:15.3 15.9mag 76P/West-Kohoutek-Ikemura
00:18:54.91 +03:56:16.4 14.6mag 78P/Gehrels
21:53:58.38 -15:34:05.0 14.5mag 88P/Howell
01:12:07.45 +14:32:53.5 15.2mag 93P/Lovas
04:17:25.55 +30:58:52.5 16.4mag 123P/West-Hartley
08:09:29.32 +48:16:00.2 16.2mag 124P/Mrkos
02:00:47.49 +11:52:59.7 16.4mag 128P/Shoemaker-Holt
02:05:51.03 +11:39:44.6 17.4mag 131P/Mueller
23:39:59.22 +04:53:35.8 12.4mag 141P/Machholz
23:50:14.04 -02:58:13.6 12.5mag 141P-A/Machholz
22:48:06.92 -05:49:36.3 15.5mag 141P-D/Machholz
00:02:43.25 -12:04:38.0 15.4mag 162P/SidingSpring
10:36:27.46 +31:58:50.2 17.6mag 164P/Christensen
05:57:25.98 +24:42:30.9 17.6mag 198P/ODAS
15:27:20.01 -02:45:38.4 17.0mag 210P/Christensen
20:28:30.34 -16:34:24.3 17.2mag 218P/LINEAR
17:03:43.78 -16:16:38.9 16.2mag 235P/LINEAR
04:50:00.03 +32:34:00.6 16.4mag 240P/NEAT
07:30:42.28 -07:46:29.0 17.5mag 242P/Spahr
15:48:13.07 +05:26:13.3 17.6mag 391P/Kowalski
07:28:28.62 +21:10:40.0 17.6mag 450P/LONEOS
05:06:25.78 +46:19:52.4 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 25 05:58 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
-rw-r--r-- 1 apache apache 5.8K Mar 25 05:58 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 25 05:58 tocp_transients_list.txt
