This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN
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
NSVS J2212515+391002,2461120.9494,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J2212515+391002 20260321.4494 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:51.18 +39:09:59.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.85 21:34:15.55 +38:14:21.3
85.73170 -10.00030 galactic Cyg Second-epoch detections are separated by 3.7" and 1.5 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 J323.5655+38.2409 | 21:34:15.55 +38:14:21.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.514+/-0.050 (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 J323.5655+38.2409,2461120.9494,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.5655+38.2409 20260321.4494 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:15.55 +38:14:21.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.85 21:32:46.01 +37:06:20.5
84.72148 -10.62021 galactic Cyg Second-epoch detections are separated by 1.9" and 1.0 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 | 21:32:46.01 +37:06:20.5 (user input) | T | P | (position from user input) J-Ks=0.194+/-0.069 (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,2461120.9494,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260321.4494 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:46.01 +37:06:20.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.78 21:45:43.36 +41:42:23.0
89.73754 -8.89312 galactic Cyg Second-epoch detections are separated by 7.6" and 0.4 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 J326.4277+41.7087 | 21:45:43.36 +41:42:23.0 (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 J326.4277+41.7087,2461120.9494,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J326.4277+41.7087 20260321.4494 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:43.36 +41:42:23.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.86 21:24:50.19 +39:27:06.1
85.24892 -7.85365 galactic Cyg Second-epoch detections are separated by 5.6" and 2.3 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 | 21:24:50.19 +39:27:06.1 (user input) | T | P | (position from user input) J-Ks=0.443+/-0.050 (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,2461120.9494,12.86,0.05,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
target 20260321.4494 12.86CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:50.19 +39:27:06.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.66 21:41:45.14 +37:40:54.2
86.45412 -11.41037 galactic Cyg Second-epoch detections are separated by 1.5" and 1.5 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 J325.4361+37.6851 | 21:41:45.14 +37:40:54.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.660+/-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 J325.4361+37.6851,2461120.9494,12.66,0.05,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 J325.4361+37.6851 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:45.14 +37:40:54.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.67 21:27:24.07 +36:58:25.0
83.84694 -9.96941 galactic Cyg Second-epoch detections are separated by 0.8" and 1.5 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 J321.8436+36.9731 | 21:27:24.07 +36:58:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.307+/-0.040 (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 J321.8436+36.9731,2461120.9494,12.67,0.05,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 J321.8436+36.9731 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:24.07 +36:58:25.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1960322927596003968,2461120.9494,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1960322927596003968 20260321.4494 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:38.29 +41:30:55.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.57 21:31:35.18 +38:09:23.1
85.28715 -9.69900 galactic Cyg Second-epoch detections are separated by 1.8" and 1.6 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 J322.9036+38.1484 | 21:31:35.18 +38:09:23.1 (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 J322.9036+38.1484,2461120.9494,12.57,0.05,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 J322.9036+38.1484 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:35.18 +38:09:23.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 J212148.15+350153.2,2461120.9494,12.44,0.05,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
ZTF J212148.15+350153.2 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:46.40 +35:01:45.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.61 21:30:47.82 +38:57:32.5
85.73675 -9.01257 galactic Cyg Second-epoch detections are separated by 1.8" and 1.7 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 J322.6994+38.9623 | 21:30:47.82 +38:57:32.5 (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 J322.6994+38.9623,2461120.9494,12.61,0.05,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 J322.6994+38.9623 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:47.82 +38:57:32.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.45 21:23:31.33 +39:22:16.0
85.01004 -7.73147 galactic Cyg Second-epoch detections are separated by 5.2" and 0.6 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 | 21:23:31.33 +39:22:16.0 (user input) | T | P | (position from user input) J-Ks=0.324+/-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
target,2461120.9494,12.45,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:31.33 +39:22:16.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.72 21:44:37.38 +38:02:19.2
87.12813 -11.52042 galactic Cyg Second-epoch detections are separated by 1.6" and 1.1 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 | 21:44:37.38 +38:02:19.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.424+/-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,2461120.9494,12.72,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:37.38 +38:02:19.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.49 21:44:52.81 +37:32:27.1
86.83089 -11.92748 galactic Cyg Second-epoch detections are separated by 0.8" and 1.3 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 J326.2183+37.5347 | 21:44:52.81 +37:32:27.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.338+/-0.042 (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 J326.2183+37.5347,2461120.9494,12.49,0.05,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 J326.2183+37.5347 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:52.81 +37:32:27.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.41 21:20:08.98 +38:06:51.3
83.64031 -8.14587 galactic Cyg Second-epoch detections are separated by 2.3" and 1.1 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 | 21:20:08.98 +38:06:51.3 (user input) | T | P | (position from user input) J-Ks=0.311+/-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
target,2461120.9494,12.41,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:08.98 +38:06:51.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.53 21:28:02.73 +38:25:44.9
84.97302 -9.02004 galactic Cyg Second-epoch detections are separated by 2.4" and 1.7 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 J322.0123+38.4340 | 21:28:02.73 +38:25:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.358+/-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 J322.0123+38.4340,2461120.9494,12.53,0.05,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 J322.0123+38.4340 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:02.73 +38:25:44.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.40 21:22:16.36 +36:13:44.9
82.57428 -9.76564 galactic Cyg Second-epoch detections are separated by 0.9" and 1.5 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 J320.5722+36.2302 | 21:22:16.36 +36:13:44.9 (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 J320.5722+36.2302,2461120.9494,12.40,0.05,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 J320.5722+36.2302 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:16.36 +36:13:44.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1949549362910257664,2461120.9494,12.34,0.05,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 1949549362910257664 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:58.95 +36:20:20.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.41 22:02:54.19 +40:52:41.4
91.74936 -11.57246 galactic Lac Second-epoch detections are separated by 1.2" and 1.2 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 | 22:02:54.19 +40:52:41.4 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.039 (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,2461120.9494,12.41,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:54.19 +40:52:41.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 J213912.00+420626.9,2461120.9494,12.46,0.05,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
ZTF J213912.00+420626.9 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:13.08 +42:06:32.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.46,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:55.94 +34:03:39.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.34 21:47:50.79 +40:31:46.2
89.26887 -10.04696 galactic Cyg Second-epoch detections are separated by 1.9" and 1.0 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 1954253829569126400 | 21:47:49.18 +40:31:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.021+/-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 1954253829569126400,2461120.9494,12.34,0.05,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 1954253829569126400 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:50.79 +40:31:46.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.40 21:34:26.75 +41:42:34.0
88.15439 -7.48817 galactic Cyg Second-epoch detections are separated by 0.7" and 1.4 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 J323.5990+41.7163 | 21:34:26.75 +41:42:34.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.505+/-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 J323.5990+41.7163,2461120.9494,12.40,0.05,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 J323.5990+41.7163 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:26.75 +41:42:34.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.22,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:52.58 +34:30:12.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.35 21:43:05.23 +41:29:28.1
89.21835 -8.73231 galactic Cyg Second-epoch detections are separated by 1.5" and 1.1 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 | 21:43:05.23 +41:29:28.1 (user input) | T | P | (position from user input) J-Ks=0.323+/-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,2461120.9494,12.35,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:05.23 +41:29:28.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.36 21:22:46.56 +34:59:22.5
81.74649 -10.70552 galactic Cyg Second-epoch detections are separated by 1.9" and 1.4 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 1855401476458121984 | 21:22:43.17 +34:59:34.1 (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 1855401476458121984,2461120.9494,12.36,0.05,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 1855401476458121984 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:46.56 +34:59:22.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.51 21:53:53.73 +41:17:51.7
90.66006 -10.18960 galactic Cyg Second-epoch detections are separated by 3.0" and 1.0 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 | 21:53:53.73 +41:17:51.7 (user input) | T | P | (position from user input) J-Ks=0.345+/-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,2461120.9494,12.51,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:53.73 +41:17:51.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.27 21:40:12.85 +36:18:00.6
85.27366 -12.22769 galactic Cyg Second-epoch detections are separated by 1.1" and 1.5 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 | Large-amplitude variable Gaia DR2 1951097200399334144 | 21:40:12.85 +36:18:00.6 (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+/-0.035 (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
Large-amplitude variable Gaia DR2 1951097200399334144,2461120.9494,12.27,0.05,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
Large-amplitude variable Gaia DR2 1951097200399334144 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:12.85 +36:18:00.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.06,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:11.65 +39:02:25.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.35 21:41:28.51 +41:30:43.6
89.00342 -8.51695 galactic Cyg Second-epoch detections are separated by 0.7" and 1.4 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 J325.3764+41.5141 | 21:41:28.51 +41:30:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.429+/-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
ATO J325.3764+41.5141,2461120.9494,12.35,0.05,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 J325.3764+41.5141 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:28.51 +41:30:43.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.14 21:27:41.77 +38:45:45.4
85.15952 -8.73384 galactic Cyg Second-epoch detections are separated by 2.3" and 1.8 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 J321.9265+38.7675 | 21:27:41.77 +38:45:45.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.638+/-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 J321.9265+38.7675,2461120.9494,12.14,0.05,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 J321.9265+38.7675 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:41.77 +38:45:45.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.18 21:19:17.68 +37:56:05.4
83.39179 -8.15008 galactic Cyg Second-epoch detections are separated by 2.4" and 1.1 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 J319.8203+37.9352 | 21:19:17.68 +37:56:05.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.740+/-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 J319.8203+37.9352,2461120.9494,12.18,0.05,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 J319.8203+37.9352 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:17.68 +37:56:05.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.25 21:44:39.07 +41:53:49.7
89.71087 -8.61823 galactic Cyg Second-epoch detections are separated by 1.8" and 1.1 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 J326.1617+41.8981 | 21:44:39.07 +41:53:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J326.1617+41.8981,2461120.9494,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J326.1617+41.8981 20260321.4494 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:39.07 +41:53:49.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.16 21:57:22.83 +40:56:51.4
90.95572 -10.87430 galactic Cyg Second-epoch detections are separated by 2.1" and 1.6 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 J329.3425+40.9483 | 21:57:22.82 +40:57:15.5 (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 J329.3425+40.9483,2461120.9494,12.16,0.05,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 J329.3425+40.9483 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:22.83 +40:56:51.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.10 21:22:31.09 +37:35:51.7
83.59821 -8.84132 galactic Cyg Second-epoch detections are separated by 3.6" and 1.6 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 J320.6269+37.5975 | 21:22:31.09 +37:35:51.7 (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 J320.6269+37.5975,2461120.9494,12.10,0.05,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 J320.6269+37.5975 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:31.09 +37:35:51.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.29 21:48:18.10 +41:54:23.7
90.23918 -9.05292 galactic Cyg Second-epoch detections are separated by 0.9" and 1.2 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 J327.0813+41.9133 | 21:48:18.10 +41:54:23.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.340+/-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
ATO J327.0813+41.9133,2461120.9494,12.29,0.05,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 J327.0813+41.9133 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:18.10 +41:54:23.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1956613381520278656,2461120.9494,12.07,0.05,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 1956613381520278656 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:59.00 +40:08:16.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.06 21:45:28.84 +42:12:24.4
90.03342 -8.48462 galactic Cyg Second-epoch detections are separated by 2.4" and 1.3 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 | 21:45:28.84 +42:12:24.4 (user input) | T | P | (position from user input) J-Ks=0.291+/-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,2461120.9494,12.06,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:28.84 +42:12:24.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1964864735256226432,2461120.9494,12.03,0.05,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
Gaia DR3 1964864735256226432 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:00.19 +38:24:37.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1951062222190619520,2461120.9494,12.01,0.05,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 1951062222190619520 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:44.95 +35:57:35.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.04 21:23:57.85 +34:02:50.2
81.23433 -11.53936 galactic Cyg Second-epoch detections are separated by 3.5" and 1.4 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 J320.9816+34.0500 | 21:23:57.85 +34:02:50.2 (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 J320.9816+34.0500,2461120.9494,12.04,0.05,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 J320.9816+34.0500 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:57.85 +34:02:50.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1855118390877000448,2461120.9494,11.96,0.05,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 1855118390877000448 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:35.29 +34:11:53.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.96 21:22:57.47 +38:21:11.6
84.20313 -8.37165 galactic Cyg Second-epoch detections are separated by 2.0" and 1.3 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 J320.7437+38.3510 | 21:22:57.47 +38:21:11.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J320.7437+38.3510,2461120.9494,11.96,0.05,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 J320.7437+38.3510 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:57.47 +38:21:11.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.92 21:31:14.96 +36:19:50.3
83.95170 -10.96865 galactic Cyg Second-epoch detections are separated by 2.0" and 1.7 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 J322.8168+36.3306 | 21:31:16.49 +36:20:06.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-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 J322.8168+36.3306,2461120.9494,11.92,0.05,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 J322.8168+36.3306 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:14.96 +36:19:50.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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
V1614 Cyg,2461120.9494,12.05,0.05,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
V1614 Cyg 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:29.29 +40:58:23.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.96 21:45:53.74 +35:13:19.2
85.41242 -13.80010 galactic Cyg Second-epoch detections are separated by 0.6" and 1.3 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 | 21:45:53.74 +35:13:19.2 (user input) | T | P | (position from user input) J-Ks=0.412+/-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,2461120.9494,11.96,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:53.74 +35:13:19.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.86 21:20:31.14 +38:20:14.1
83.85270 -8.04207 galactic Cyg Second-epoch detections are separated by 1.5" and 1.5 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 J320.1301+38.3400 | 21:20:31.14 +38:20:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.522+/-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 J320.1301+38.3400,2461120.9494,11.86,0.05,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
ATO J320.1301+38.3400 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:31.14 +38:20:14.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.90 21:20:26.99 +35:31:37.1
81.80203 -9.99047 galactic Cyg Second-epoch detections are separated by 1.5" and 1.2 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 | 21:20:26.99 +35:31:37.1 (user input) | T | P | (position from user input) J-Ks=0.735+/-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
target,2461120.9494,11.90,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:26.99 +35:31:37.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.87 21:32:48.46 +39:29:41.6
86.39625 -8.89272 galactic Cyg Second-epoch detections are separated by 2.0" and 1.7 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 J323.2117+39.4959 | 21:32:48.46 +39:29:41.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.412+/-0.044 (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 J323.2117+39.4959,2461120.9494,11.87,0.05,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 J323.2117+39.4959 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:48.46 +39:29:41.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1947972353997813376,2461120.9494,11.93,0.05,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 1947972353997813376 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:37.13 +33:56:11.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.88 21:19:18.67 +37:19:00.9
82.94518 -8.58205 galactic Cyg Second-epoch detections are separated by 1.6" and 1.5 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 | Gaia DR3 1963961275989904128 | 21:19:19.51 +37:19:20.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-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
Gaia DR3 1963961275989904128,2461120.9494,11.88,0.05,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
Gaia DR3 1963961275989904128 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:18.67 +37:19:00.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1964854770931615872,2461120.9494,11.79,0.05,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 1964854770931615872 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:47.35 +38:10:22.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.53 21:26:04.93 +37:38:02.0
84.12883 -9.31554 galactic Cyg Second-epoch detections are separated by 2.4" and 1.1 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 J321.5250+37.6297 | 21:26:04.93 +37:38:02.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.402+/-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
ATO J321.5250+37.6297,2461120.9494,11.53,0.05,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
ATO J321.5250+37.6297 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:04.93 +37:38:02.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.57 21:22:26.13 +37:11:04.3
83.28857 -9.11960 galactic Cyg Second-epoch detections are separated by 0.6" and 1.5 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 J320.6100+37.1872 | 21:22:26.13 +37:11:04.3 (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 J320.6100+37.1872,2461120.9494,11.57,0.05,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 J320.6100+37.1872 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:26.13 +37:11:04.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.59 21:19:57.19 +39:52:25.7
84.88332 -6.88931 galactic Cyg Second-epoch detections are separated by 2.5" and 1.0 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 J319.9852+39.8763 | 21:19:57.19 +39:52:25.7 (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 J319.9852+39.8763,2461120.9494,11.59,0.05,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
ATO J319.9852+39.8763 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:57.19 +39:52:25.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.57 22:00:14.39 +41:40:34.0
91.84415 -10.63521 galactic Lac Second-epoch detections are separated by 1.4" and 1.5 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 J330.0567+41.6700 | 22:00:14.39 +41:40:34.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J330.0567+41.6700,2461120.9494,11.57,0.05,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 J330.0567+41.6700 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:14.39 +41:40:34.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.50 21:55:20.92 +40:52:13.1
90.60187 -10.69395 galactic Cyg Second-epoch detections are separated by 0.9" and 1.2 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 J328.8488+40.8741 | 21:55:20.92 +40:52:13.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.478+/-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 J328.8488+40.8741,2461120.9494,11.50,0.05,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
ATO J328.8488+40.8741 20260321.4494 11.50CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:20.92 +40:52:13.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.57 22:13:41.76 +40:56:39.1
93.46646 -12.73191 galactic Lac Second-epoch detections are separated by 1.8" and 1.5 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 J333.4332+40.9387 | 22:13:41.76 +40:56:39.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.323+/-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 J333.4332+40.9387,2461120.9494,11.57,0.05,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 J333.4332+40.9387 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:41.76 +40:56:39.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.46 21:28:47.08 +42:05:19.1
87.64483 -6.48934 galactic Cyg Second-epoch detections are separated by 1.2" and 1.5 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 | 21:28:47.08 +42:05:19.1 (user input) | T | P | (position from user input) J-Ks=0.784+/-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
target,2461120.9494,11.46,0.05,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 20260321.4494 11.46CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:47.08 +42:05:19.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.36 21:51:52.25 +41:19:33.8
90.38010 -9.92623 galactic Cyg Second-epoch detections are separated by 0.4" and 1.3 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 | 21:51:52.25 +41:19:33.8 (user input) | T | P | (position from user input) J-Ks=0.423+/-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,2461120.9494,11.36,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:52.25 +41:19:33.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1964745159067548800,2461120.9494,11.32,0.05,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 1964745159067548800 20260321.4494 11.32CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:16.76 +37:55:32.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.17 21:28:09.28 +41:14:36.0
86.96883 -7.01634 galactic Cyg Second-epoch detections are separated by 1.6" and 1.2 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 J322.0200+41.2443 | 21:28:07.89 +41:14:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.370+/-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 J322.0200+41.2443,2461120.9494,11.17,0.05,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 J322.0200+41.2443 20260321.4494 11.17CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:09.28 +41:14:36.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.01 21:18:26.49 +38:35:23.1
83.74953 -7.57442 galactic Cyg Second-epoch detections are separated by 0.4" and 1.3 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 1964913800964183680 | 21:18:29.36 +38:34:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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
Gaia DR3 1964913800964183680,2461120.9494,11.01,0.05,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
Gaia DR3 1964913800964183680 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:26.49 +38:35:23.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.07 21:54:25.00 +39:39:27.7
89.68085 -11.52175 galactic Cyg Second-epoch detections are separated by 0.9" and 1.2 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 1959168337307618304 | 21:54:23.59 +39:39:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.125+/-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 1959168337307618304,2461120.9494,11.07,0.05,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 1959168337307618304 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:25.00 +39:39:27.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.06 21:46:27.10 +42:00:03.0
90.03590 -8.75820 galactic Cyg Second-epoch detections are separated by 0.9" and 1.2 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 | 21:46:27.10 +42:00:03.0 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.741+/-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,2461120.9494,11.06,0.05,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
target 20260321.4494 11.06CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:27.10 +42:00:03.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 10.67 21:31:37.92 +34:11:28.6
82.48705 -12.55834 galactic Cyg Second-epoch detections are separated by 0.6" and 1.4 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 J322.9137+34.1966 | 21:31:37.92 +34:11:28.6 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.487+/-0.024 (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 J322.9137+34.1966,2461120.9494,10.67,0.05,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 J322.9137+34.1966 20260321.4494 10.67CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:37.92 +34:11:28.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 9.91 21:23:53.58 +35:33:45.7
82.32506 -10.46680 galactic Cyg Second-epoch detections are separated by 1.2" and 1.5 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 J320.9777+35.5618 | 21:23:54.44 +35:34:01.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.232+/-0.025 (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 J320.9777+35.5618,2461120.9494,9.91,0.05,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 J320.9777+35.5618 20260321.4494 9.91CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:53.58 +35:33:45.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 9.96 21:24:39.85 +33:48:21.5
81.16221 -11.81199 galactic Cyg Second-epoch detections are separated by 0.1" and 1.5 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 | NSV 13690 | 21:24:36.99 +33:48:21.1 (Gaia DR3) | (local) | A0 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.840+/-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
NSV 13690,2461120.9494,9.96,0.05,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
NSV 13690 20260321.4494 9.96CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:39.85 +33:48:21.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 10.29 21:39:25.90 +41:43:13.8
88.85560 -8.10718 galactic Cyg Second-epoch detections are separated by 2.0" and 1.4 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 1966523657783024640 | 21:39:28.73 +41:43:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G9V 1950ApJ...111..221W HD 206224
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1966523657783024640,2461120.9494,10.29,0.05,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
Gaia DR3 1966523657783024640 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:25.90 +41:43:13.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 10.52 21:47:57.33 +36:35:33.9
86.66427 -13.04496 galactic Cyg Second-epoch detections are separated by 0.4" and 1.4 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 1952454543207886464 | 21:47:57.30 +36:35:34.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.751+/-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 1952454543207886464,2461120.9494,10.52,0.05,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
Gaia DR3 1952454543207886464 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:57.33 +36:35:33.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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
V1907 Cyg,2461120.9494,10.66,0.05,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
V1907 Cyg 20260321.4494 10.66CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:14.81 +39:26:58.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 10.67 21:42:55.14 +41:10:20.0
88.98136 -8.95110 galactic Cyg Second-epoch detections are separated by 0.4" and 1.3 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 1954518120374734464 | 21:42:55.04 +41:10:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.059+/-0.044 (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 1954518120374734464,2461120.9494,10.67,0.05,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
Gaia DR3 1954518120374734464 20260321.4494 10.67CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:55.14 +41:10:20.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1952708225458525824,2461120.9494,10.75,0.05,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
Gaia DR3 1952708225458525824 20260321.4494 10.75CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:50.27 +37:29:32.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.00 21:27:46.08 +35:33:54.1
82.89322 -11.02307 galactic Cyg Second-epoch detections are separated by 0.2" and 1.5 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 | 21:27:46.08 +35:33:54.1 (user input) | T | P | (position from user input) J-Ks=0.359+/-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,2461120.9494,11.00,0.05,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
target 20260321.4494 11.00CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:46.08 +35:33:54.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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
V1338 Cyg,2461120.9494,11.08,0.05,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
V1338 Cyg 20260321.4494 11.08CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:04.78 +40:51:23.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.12 22:08:33.83 +41:26:35.6
92.96554 -11.76160 galactic Lac Second-epoch detections are separated by 0.4" and 1.4 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 J332.1391+41.4415 | 22:08:33.83 +41:26:35.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.428+/-0.044 (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 J332.1391+41.4415,2461120.9494,11.12,0.05,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 J332.1391+41.4415 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:33.83 +41:26:35.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.22 21:52:09.56 +38:58:10.1
88.88948 -11.77380 galactic Cyg Second-epoch detections are separated by 0.6" and 1.2 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 | 21:52:09.56 +38:58:10.1 (user input) | T | P | (position from user input) J-Ks=0.770+/-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,2461120.9494,11.22,0.05,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 20260321.4494 11.22CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:09.56 +38:58:10.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,11.21,0.05,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
target 20260321.4494 11.21CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:48.44 +41:41:43.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.33 21:39:05.39 +36:51:24.2
85.48779 -11.66482 galactic Cyg Second-epoch detections are separated by 0.4" and 1.4 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 1951171241339527424 | 21:39:03.98 +36:52:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.402+/-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
Gaia DR3 1951171241339527424,2461120.9494,11.33,0.05,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
Gaia DR3 1951171241339527424 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:05.39 +36:51:24.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.30 22:13:14.65 +41:47:42.9
93.90057 -11.98917 galactic Lac Second-epoch detections are separated by 0.5" and 1.3 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 J333.2961+41.7989 | 22:13:14.65 +41:47:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.941+/-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 J333.2961+41.7989,2461120.9494,11.30,0.05,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 J333.2961+41.7989 20260321.4494 11.30CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:14.65 +41:47:42.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.29 21:56:37.89 +37:20:32.3
88.52246 -13.58825 galactic Cyg Second-epoch detections are separated by 1.3" and 1.4 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 J329.1389+37.3457 | 21:56:35.79 +37:20:59.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.557+/-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 J329.1389+37.3457,2461120.9494,11.29,0.05,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 J329.1389+37.3457 20260321.4494 11.29CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:37.89 +37:20:32.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.25 21:33:36.34 +38:32:50.2
85.85143 -9.68827 galactic Cyg Second-epoch detections are separated by 0.9" and 1.2 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 | 21:33:36.34 +38:32:50.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.285+/-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,2461120.9494,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260321.4494 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:36.34 +38:32:50.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1955258748835187456,2461120.9494,11.43,0.05,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 1955258748835187456 20260321.4494 11.43CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:58.64 +38:26:20.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.34 21:18:40.03 +39:14:36.1
84.25400 -7.15155 galactic Cyg Second-epoch detections are separated by 1.6" and 1.7 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 1965155379979232000 | 21:18:40.87 +39:14:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-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 1965155379979232000,2461120.9494,11.34,0.05,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 1965155379979232000 20260321.4494 11.34CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:40.03 +39:14:36.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.41 21:41:29.15 +37:46:45.6
86.48075 -11.30256 galactic Cyg Second-epoch detections are separated by 0.4" and 1.4 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 J325.3761+37.7784 | 21:41:29.15 +37:46:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.363+/-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 J325.3761+37.7784,2461120.9494,11.41,0.05,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 J325.3761+37.7784 20260321.4494 11.41CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:29.15 +37:46:45.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.43 21:32:54.35 +35:30:10.4
83.61223 -11.79745 galactic Cyg Second-epoch detections are separated by 1.5" and 1.2 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 1951363316579121152 | 21:32:51.70 +35:29:57.4 (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 1951363316579121152,2461120.9494,11.43,0.05,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 1951363316579121152 20260321.4494 11.43CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:54.35 +35:30:10.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.58 21:20:46.72 +33:50:41.5
80.61702 -11.20595 galactic Cyg Second-epoch detections are separated by 2.3" and 1.5 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 J320.1900+33.8436 | 21:20:46.72 +33:50:41.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.321+/-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 J320.1900+33.8436,2461120.9494,11.58,0.05,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 J320.1900+33.8436 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:46.72 +33:50:41.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.48 21:39:07.89 +36:52:27.7
85.50623 -11.65746 galactic Cyg Second-epoch detections are separated by 2.0" and 1.2 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 J324.7925+36.8647 | 21:39:07.89 +36:52:27.7 (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 J324.7925+36.8647,2461120.9494,11.48,0.05,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
ATO J324.7925+36.8647 20260321.4494 11.48CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:07.89 +36:52:27.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.55 22:07:50.36 +40:07:28.2
92.04955 -12.73966 galactic Lac Second-epoch detections are separated by 0.8" and 1.2 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 J331.9519+40.1216 | 22:07:50.36 +40:07:28.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.493+/-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 J331.9519+40.1216,2461120.9494,11.55,0.05,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 J331.9519+40.1216 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:50.36 +40:07:28.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.57 21:48:53.62 +40:38:12.4
89.49329 -10.09399 galactic Cyg Second-epoch detections are separated by 0.9" and 1.3 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 J327.2219+40.6351 | 21:48:53.62 +40:38:12.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.436+/-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 J327.2219+40.6351,2461120.9494,11.57,0.05,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 J327.2219+40.6351 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:53.62 +40:38:12.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1964843947614126976,2461120.9494,11.55,0.05,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 1964843947614126976 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:36.10 +38:11:41.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.54 21:35:30.51 +34:46:53.2
83.49629 -12.68668 galactic Cyg Second-epoch detections are separated by 0.9" and 1.5 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 | 21:35:30.51 +34:46:53.2 (user input) | T | P | (position from user input) J-Ks=0.777+/-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,2461120.9494,11.54,0.05,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 20260321.4494 11.54CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:30.51 +34:46:53.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.55 21:22:57.16 +34:21:06.6
81.30744 -11.17693 galactic Cyg Second-epoch detections are separated by 0.7" and 1.5 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 | Gaia DR3 1855344649753169280 | 21:22:54.85 +34:21:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.401+/-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
Gaia DR3 1855344649753169280,2461120.9494,11.55,0.05,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 1855344649753169280 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:57.16 +34:21:06.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.56 21:55:05.31 +34:46:30.7
86.58441 -15.36767 galactic Peg Second-epoch detections are separated by 0.8" and 1.4 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 | 21:55:05.31 +34:46:30.7 (user input) | T | P | (position from user input) J-Ks=0.439+/-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,2461120.9494,11.56,0.05,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 20260321.4494 11.56CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:05.31 +34:46:30.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,11.59,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:07.76 +38:56:42.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.61 22:01:49.89 +36:55:26.7
89.08533 -14.56342 galactic Lac Second-epoch detections are separated by 3.0" and 1.6 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 | 22:01:49.89 +36:55:26.7 (user input) | T | P | (position from user input) J-Ks=0.286+/-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
target,2461120.9494,11.61,0.05,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 20260321.4494 11.61CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:49.89 +36:55:26.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.62 22:06:46.19 +39:39:09.6
91.59103 -12.99441 galactic Lac Second-epoch detections are separated by 0.3" and 1.3 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 | 22:06:46.19 +39:39:09.6 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461120.9494,11.62,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:46.19 +39:39:09.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.62 21:42:50.12 +38:10:45.9
86.95485 -11.18189 galactic Cyg Second-epoch detections are separated by 1.0" and 1.2 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 J325.6987+38.1778 | 21:42:50.12 +38:10:45.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.374+/-0.041 (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 J325.6987+38.1778,2461120.9494,11.62,0.05,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 J325.6987+38.1778 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:50.12 +38:10:45.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.63 21:42:06.19 +36:50:53.8
85.93772 -12.07661 galactic Cyg Second-epoch detections are separated by 0.4" and 1.4 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 J325.5190+36.8572 | 21:42:06.19 +36:50:53.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.352+/-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 J325.5190+36.8572,2461120.9494,11.63,0.05,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 J325.5190+36.8572 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:06.19 +36:50:53.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.69 22:11:23.05 +39:44:15.2
92.37585 -13.45417 galactic Lac Second-epoch detections are separated by 0.3" and 1.3 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 | 22:11:23.05 +39:44:15.2 (user input) | T | P | (position from user input) J-Ks=0.721+/-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,2461120.9494,11.69,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:23.05 +39:44:15.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,11.58,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:53.38 +34:58:18.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.79 22:13:05.31 +41:48:40.8
93.88593 -11.95925 galactic Lac Second-epoch detections are separated by 1.3" and 1.5 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 | 22:13:05.31 +41:48:40.8 (user input) | T | P | (position from user input) J-Ks=0.719+/-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,2461120.9494,11.79,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:05.31 +41:48:40.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.80 22:00:54.57 +41:16:15.2
91.69128 -11.03194 galactic Lac Second-epoch detections are separated by 1.1" and 1.3 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 | 22:00:54.57 +41:16:15.2 (user input) | T | P | (position from user input) J-Ks=0.301+/-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
target,2461120.9494,11.80,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:54.57 +41:16:15.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260321.4494 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:21.28 +34:05:46.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.89 21:39:20.65 +35:38:18.7
84.68271 -12.59601 galactic Cyg Second-epoch detections are separated by 0.5" and 1.3 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 | 21:39:20.65 +35:38:18.7 (user input) | T | P | (position from user input) J-Ks=0.552+/-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,2461120.9494,11.89,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:20.65 +35:38:18.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.89 21:44:49.77 +36:56:55.7
86.42228 -12.36457 galactic Cyg Second-epoch detections are separated by 1.3" and 1.5 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 | 21:44:49.77 +36:56:55.7 (user input) | T | P | (position from user input) J-Ks=0.402+/-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
target,2461120.9494,11.89,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:49.77 +36:56:55.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.81 21:49:54.58 +34:54:44.0
85.83901 -14.57438 galactic Peg Second-epoch detections are separated by 0.9" and 1.3 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 | 21:49:54.58 +34:54:44.0 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.040 (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,2461120.9494,11.81,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:54.58 +34:54:44.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.82 21:50:52.30 +39:37:43.0
89.12623 -11.10846 galactic Cyg Second-epoch detections are separated by 0.9" and 1.2 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 J327.7283+39.6224 | 21:50:52.30 +39:37:43.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.697+/-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 J327.7283+39.6224,2461120.9494,11.82,0.05,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 J327.7283+39.6224 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:52.30 +39:37:43.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,11.81,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:00.09 +39:46:41.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.91 22:21:21.26 +41:17:36.3
94.88810 -13.26429 galactic Lac Second-epoch detections are separated by 0.7" and 1.2 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 J335.3499+41.2971 | 22:21:21.26 +41:17:36.3 (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 J335.3499+41.2971,2461120.9494,11.91,0.05,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 J335.3499+41.2971 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:21.26 +41:17:36.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.97 21:23:19.64 +35:13:30.0
81.99794 -10.62141 galactic Cyg Second-epoch detections are separated by 0.8" and 1.3 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 J320.8355+35.2221 | 21:23:19.64 +35:13:30.0 (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 J320.8355+35.2221,2461120.9494,11.97,0.05,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 J320.8355+35.2221 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:19.64 +35:13:30.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.96 22:16:38.13 +41:45:37.6
94.40953 -12.38091 galactic Lac Second-epoch detections are separated by 2.1" and 1.0 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 J334.1643+41.7554 | 22:16:38.13 +41:45:37.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.547+/-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 J334.1643+41.7554,2461120.9494,11.96,0.05,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 J334.1643+41.7554 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:38.13 +41:45:37.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.85 22:02:40.25 +38:06:45.2
89.97737 -13.73157 galactic Lac Second-epoch detections are separated by 0.7" and 1.4 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 J330.6734+38.1123 | 22:02:40.25 +38:06:45.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.372+/-0.064 (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 J330.6734+38.1123,2461120.9494,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J330.6734+38.1123 20260321.4494 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:40.25 +38:06:45.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,11.91,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:02.61 +37:17:54.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.13 22:13:03.63 +38:28:17.9
91.88068 -14.66972 galactic Lac Second-epoch detections are separated by 1.2" and 1.1 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 | 22:13:03.63 +38:28:17.9 (user input) | T | P | (position from user input) J-Ks=0.384+/-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,2461120.9494,12.13,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:03.63 +38:28:17.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.92 21:39:39.54 +39:57:28.3
87.69481 -9.44611 galactic Cyg Second-epoch detections are separated by 1.0" and 1.3 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 J324.9057+39.9504 | 21:39:39.54 +39:57:28.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.436+/-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 J324.9057+39.9504,2461120.9494,11.92,0.05,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 J324.9057+39.9504 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:39.54 +39:57:28.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.99 21:21:16.92 +34:59:15.3
81.52800 -10.48755 galactic Cyg Second-epoch detections are separated by 1.2" and 1.5 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 | 21:21:16.92 +34:59:15.3 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.039 (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,2461120.9494,11.99,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:16.92 +34:59:15.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.94 21:57:20.62 +40:57:00.4
90.95177 -10.86800 galactic Cyg Second-epoch detections are separated by 1.5" and 1.6 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 J329.3425+40.9483 | 21:57:22.82 +40:57:15.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.451+/-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 J329.3425+40.9483,2461120.9494,11.94,0.05,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
ATO J329.3425+40.9483 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:20.62 +40:57:00.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.01 22:06:31.79 +34:33:33.0
88.34969 -17.01298 galactic Peg Second-epoch detections are separated by 3.0" and 0.9 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 | 22:06:31.79 +34:33:33.0 (user input) | T | P | (position from user input) J-Ks=0.631+/-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,2461120.9494,12.01,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:31.79 +34:33:33.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.74 21:27:05.58 +36:00:32.0
83.11248 -10.61152 galactic Cyg Second-epoch detections are separated by 1.9" and 1.7 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 J321.7704+36.0100 | 21:27:03.84 +36:00:00.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.442+/-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 J321.7704+36.0100,2461120.9494,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.7704+36.0100 20260321.4494 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:05.58 +36:00:32.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.90 21:20:36.26 +35:29:43.0
81.80106 -10.03511 galactic Cyg Second-epoch detections are separated by 3.1" and 1.0 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 1867486453581738880 | 21:20:36.48 +35:28:58.8 (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 1867486453581738880,2461120.9494,11.90,0.05,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
Gaia DR3 1867486453581738880 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:36.26 +35:29:43.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.95 21:36:04.29 +41:56:44.6
88.54050 -7.51979 galactic Cyg Second-epoch detections are separated by 2.4" and 1.3 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 J324.0150+41.9494 | 21:36:04.29 +41:56:44.6 (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 J324.0150+41.9494,2461120.9494,11.95,0.05,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 J324.0150+41.9494 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:04.29 +41:56:44.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.89 21:54:04.37 +37:39:41.1
88.32825 -13.01936 galactic Cyg Second-epoch detections are separated by 1.6" and 1.2 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 J328.5216+37.6572 | 21:54:04.06 +37:39:00.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5) J-Ks=0.719+/-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 J328.5216+37.6572,2461120.9494,11.89,0.05,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
ATO J328.5216+37.6572 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:04.37 +37:39:41.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.97 21:52:31.17 +41:28:58.3
90.57666 -9.88277 galactic Cyg Second-epoch detections are separated by 2.0" and 1.0 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 1960357802729664512 | 21:52:34.39 +41:28:42.5 (Gaia DR3) | ROT (local) | (local) | 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 1960357802729664512,2461120.9494,11.97,0.05,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 1960357802729664512 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:31.17 +41:28:58.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.90 21:43:16.93 +40:27:46.9
88.55915 -9.52904 galactic Cyg Second-epoch detections are separated by 1.4" and 1.5 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 | 21:43:16.93 +40:27:46.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461120.9494,11.90,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:16.93 +40:27:46.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1953796913770434944,2461120.9494,11.94,0.05,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 1953796913770434944 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:06.90 +38:39:19.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.10 22:02:27.76 +42:04:01.6
92.42055 -10.57922 galactic Lac Second-epoch detections are separated by 1.0" and 1.2 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 J330.6159+42.0668 | 22:02:27.76 +42:04:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.428+/-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 J330.6159+42.0668,2461120.9494,12.10,0.05,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 J330.6159+42.0668 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:27.76 +42:04:01.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.11 21:18:30.05 +39:08:10.7
84.15389 -7.20287 galactic Cyg Second-epoch detections are separated by 3.0" and 1.9 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 1965153318394943360 | 21:18:29.76 +39:07:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.323+/-0.041 (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 1965153318394943360,2461120.9494,12.11,0.05,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
Gaia DR3 1965153318394943360 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:30.05 +39:08:10.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1949071109713094272,2461120.9494,12.04,0.05,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 1949071109713094272 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:11.57 +35:33:08.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.04 21:38:09.28 +38:56:17.1
86.78098 -10.00562 galactic Cyg Second-epoch detections are separated by 1.1" and 1.2 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 J324.5358+38.9323 | 21:38:09.28 +38:56:17.1 (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 J324.5358+38.9323,2461120.9494,12.04,0.05,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 J324.5358+38.9323 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:09.28 +38:56:17.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.04 22:09:46.26 +41:39:58.4
93.28623 -11.71525 galactic Lac Second-epoch detections are separated by 1.1" and 1.1 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 1958254196465679360 | 22:09:49.52 +41:39:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-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 1958254196465679360,2461120.9494,12.04,0.05,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 1958254196465679360 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:46.26 +41:39:58.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.97 21:27:48.41 +38:33:03.8
85.02548 -8.90021 galactic Cyg Second-epoch detections are separated by 2.8" and 1.6 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 J321.9445+38.5586 | 21:27:46.69 +38:33:31.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE 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
ATO J321.9445+38.5586,2461120.9494,11.97,0.05,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 J321.9445+38.5586 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:48.41 +38:33:03.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.96 21:46:21.76 +39:50:08.5
88.59113 -10.38873 galactic Cyg Second-epoch detections are separated by 1.2" and 1.2 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 | 21:46:21.76 +39:50:08.5 (user input) | T | P | (position from user input) J-Ks=0.451+/-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,2461120.9494,11.96,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:21.76 +39:50:08.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.89 21:49:12.20 +34:20:08.5
85.33449 -14.91416 galactic Cyg Second-epoch detections are separated by 2.4" and 1.1 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 | 21:49:12.20 +34:20:08.5 (user input) | T | P | (position from user input) J-Ks=0.543+/-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,2461120.9494,11.89,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:12.20 +34:20:08.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 11.99 21:21:51.04 +37:53:26.0
83.71562 -8.54181 galactic Cyg Second-epoch detections are separated by 1.5" and 1.3 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 1964072674567131520 | 21:21:52.25 +37:52:56.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.459+/-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
Gaia DR3 1964072674567131520,2461120.9494,11.99,0.05,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 1964072674567131520 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:51.04 +37:53:26.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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
V1616 Cyg,2461120.9494,12.05,0.05,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
V1616 Cyg 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:09.87 +36:39:08.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.11 21:43:32.06 +38:44:15.1
87.43655 -10.85531 galactic Cyg Second-epoch detections are separated by 0.3" and 1.4 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 1953638957749125248 | 21:43:30.75 +38:43:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.382+/-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
Gaia DR3 1953638957749125248,2461120.9494,12.11,0.05,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
Gaia DR3 1953638957749125248 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:32.06 +38:44:15.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.18 21:43:30.47 +41:30:12.3
89.28648 -8.77498 galactic Cyg Second-epoch detections are separated by 1.3" and 1.2 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 | 21:43:30.47 +41:30:12.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461120.9494,12.18,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:30.47 +41:30:12.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1963590882313545216,2461120.9494,12.04,0.05,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 1963590882313545216 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:07.84 +36:03:45.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.05 21:49:54.43 +37:45:56.6
87.75066 -12.40933 galactic Cyg Second-epoch detections are separated by 0.9" and 1.5 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 | 21:49:54.43 +37:45:56.6 (user input) | T | P | (position from user input) J-Ks=0.468+/-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
target,2461120.9494,12.05,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:54.43 +37:45:56.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.06 21:34:12.43 +39:03:18.4
86.29078 -9.39860 galactic Cyg Second-epoch detections are separated by 2.3" and 1.6 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 | ASASSN-V J213414.64+390328.0 | 21:34:14.70 +39:03:29.1 (Gaia DR3) | YSO (local) | d (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.949+/-0.041 (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
ASASSN-V J213414.64+390328.0,2461120.9494,12.06,0.05,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
ASASSN-V J213414.64+390328.0 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:12.43 +39:03:18.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.09 21:57:34.03 +41:27:52.3
91.31155 -10.49197 galactic Cyg Second-epoch detections are separated by 1.3" and 1.5 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 | 21:57:34.03 +41:27:52.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.410+/-0.059 (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,2461120.9494,12.09,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:34.03 +41:27:52.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.03 21:39:00.67 +38:41:34.2
86.73820 -10.29923 galactic Cyg Second-epoch detections are separated by 1.5" and 1.4 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 J324.7488+38.6969 | 21:38:58.77 +38:41:57.6 (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 J324.7488+38.6969,2461120.9494,12.03,0.05,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 J324.7488+38.6969 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:00.67 +38:41:34.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1964626141231455232,2461120.9494,12.13,0.05,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
Gaia DR3 1964626141231455232 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:29.31 +39:08:36.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.16,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:11.32 +39:28:34.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.11 21:58:43.28 +42:11:58.3
91.94644 -10.04905 galactic Lac Second-epoch detections are separated by 0.4" and 1.3 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 J329.6664+42.1926 | 21:58:43.28 +42:11:58.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.761+/-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 J329.6664+42.1926,2461120.9494,12.11,0.05,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 J329.6664+42.1926 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:43.28 +42:11:58.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.14 22:05:42.75 +35:53:01.3
89.05843 -15.86399 galactic Lac Second-epoch detections are separated by 1.7" and 1.2 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 J331.4278+35.8836 | 22:05:42.75 +35:53:01.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.451+/-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 J331.4278+35.8836,2461120.9494,12.14,0.05,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 J331.4278+35.8836 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:42.75 +35:53:01.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.01 21:51:54.98 +33:54:39.2
85.48603 -15.60288 galactic Peg Second-epoch detections are separated by 1.7" and 1.1 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 J327.9821+33.9286 | 21:51:55.70 +33:55:11.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.455+/-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 J327.9821+33.9286,2461120.9494,12.01,0.05,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 J327.9821+33.9286 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:54.98 +33:54:39.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.10 21:56:45.17 +36:22:45.2
87.91314 -14.34883 galactic Peg Second-epoch detections are separated by 1.2" and 1.2 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 1949553108124314496 | 21:56:43.21 +36:23:14.5 (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 1949553108124314496,2461120.9494,12.10,0.05,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
Gaia DR3 1949553108124314496 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:45.17 +36:22:45.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.07 21:32:57.30 +38:12:17.6
85.51870 -9.84941 galactic Cyg Second-epoch detections are separated by 1.0" and 1.5 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 | ASASSN-V J213300.44+381231.7 | 21:33:00.44 +38:12:31.7 (Gaia DR3) | L (local) | (local) | 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
ASASSN-V J213300.44+381231.7,2461120.9494,12.07,0.05,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
ASASSN-V J213300.44+381231.7 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:57.30 +38:12:17.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1951993886497805696,2461120.9494,12.16,0.05,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 1951993886497805696 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:34.05 +37:11:49.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.06 22:13:03.64 +38:27:56.2
91.87705 -14.67462 galactic Lac Second-epoch detections are separated by 0.4" and 1.3 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 | 22:13:03.64 +38:27:56.2 (user input) | T | P | (position from user input) J-Ks=0.456+/-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,2461120.9494,12.06,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:03.64 +38:27:56.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.09 21:40:39.17 +41:35:37.9
88.94207 -8.35364 galactic Cyg Second-epoch detections are separated by 0.2" and 1.4 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 1966600378778985856 | 21:40:41.65 +41:35:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-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 1966600378778985856,2461120.9494,12.09,0.05,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 1966600378778985856 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:39.17 +41:35:37.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.11 21:29:19.08 +40:28:36.3
86.59187 -7.72081 galactic Cyg Second-epoch detections are separated by 1.8" and 1.1 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 J322.3304+40.4753 | 21:29:19.08 +40:28:36.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.370+/-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 J322.3304+40.4753,2461120.9494,12.11,0.05,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 J322.3304+40.4753 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:19.08 +40:28:36.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1955512632942240128,2461120.9494,12.12,0.05,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 1955512632942240128 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:10:19.95 +38:44:17.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.11 21:31:28.76 +34:33:30.8
82.72637 -12.27328 galactic Cyg Second-epoch detections are separated by 1.3" and 1.4 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 | 21:31:28.76 +34:33:30.8 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.026 (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,2461120.9494,12.11,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:28.76 +34:33:30.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.20 22:15:17.59 +39:47:56.7
93.04086 -13.84198 galactic Lac Second-epoch detections are separated by 1.9" and 1.2 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 | 22:15:17.59 +39:47:56.7 (user input) | T | P | (position from user input) J-Ks=0.376+/-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,2461120.9494,12.20,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:17.59 +39:47:56.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.09 21:23:16.30 +35:12:48.0
81.98136 -10.62146 galactic Cyg Second-epoch detections are separated by 1.0" and 1.5 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 | 21:23:16.30 +35:12:48.0 (user input) | T | P | (position from user input) J-Ks=0.469+/-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,2461120.9494,12.09,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:16.30 +35:12:48.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.12 21:30:29.32 +34:39:52.2
82.65289 -12.05507 galactic Cyg Second-epoch detections are separated by 0.6" and 1.4 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 J322.6185+34.6631 | 21:30:29.32 +34:39:52.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.336+/-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 J322.6185+34.6631,2461120.9494,12.12,0.05,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 J322.6185+34.6631 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:29.32 +34:39:52.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.19 21:58:13.58 +38:26:16.0
89.48210 -12.93508 galactic Lac Second-epoch detections are separated by 0.6" and 1.3 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 J329.5804+38.4365 | 21:58:17.35 +38:26:11.2 (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 J329.5804+38.4365,2461120.9494,12.19,0.05,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 J329.5804+38.4365 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:13.58 +38:26:16.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.13,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:06.03 +34:59:43.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1956026134933788544,2461120.9494,12.23,0.05,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 1956026134933788544 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:00.17 +38:42:22.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.35,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:36.46 +37:39:35.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.27 21:36:02.24 +39:50:06.7
87.09126 -9.06832 galactic Cyg Second-epoch detections are separated by 0.6" and 1.5 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 J324.0118+39.8383 | 21:36:02.24 +39:50:06.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.476+/-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 J324.0118+39.8383,2461120.9494,12.27,0.05,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 J324.0118+39.8383 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:02.24 +39:50:06.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.14 21:25:10.35 +36:09:27.9
82.94020 -10.23204 galactic Cyg Second-epoch detections are separated by 3.4" and 1.8 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 J321.2945+36.1773 | 21:25:09.32 +36:10:10.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.351+/-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 J321.2945+36.1773,2461120.9494,12.14,0.05,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 J321.2945+36.1773 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:10.35 +36:09:27.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.27 22:18:15.73 +40:51:52.2
94.14521 -13.29173 galactic Lac Second-epoch detections are separated by 2.5" and 1.4 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 1957268965327159552 | 22:18:16.91 +40:51:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-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
Gaia DR3 1957268965327159552,2461120.9494,12.27,0.05,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 1957268965327159552 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:15.73 +40:51:52.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.20 21:38:38.15 +33:58:30.9
83.41102 -13.71595 galactic Cyg Second-epoch detections are separated by 1.0" and 1.3 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 | 21:38:38.15 +33:58:30.9 (user input) | T | P | (position from user input) J-Ks=0.438+/-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,2461120.9494,12.20,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:38.15 +33:58:30.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.16 21:57:15.92 +39:56:53.4
90.30138 -11.64081 galactic Cyg Second-epoch detections are separated by 3.4" and 1.3 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 J329.3164+39.9493 | 21:57:15.92 +39:56:53.4 (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 J329.3164+39.9493,2461120.9494,12.16,0.05,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 J329.3164+39.9493 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:15.92 +39:56:53.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.21 21:58:15.48 +41:40:34.6
91.54832 -10.40642 galactic Lac Second-epoch detections are separated by 0.9" and 1.4 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 | 21:58:15.48 +41:40:34.6 (user input) | T | P | (position from user input) J-Ks=0.255+/-0.040 (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,2461120.9494,12.21,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:15.48 +41:40:34.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1953651984391739904,2461120.9494,12.30,0.05,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
Gaia DR3 1953651984391739904 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:29.72 +38:25:54.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.30 22:06:29.39 +39:42:25.0
91.58038 -12.91864 galactic Lac Second-epoch detections are separated by 1.8" and 1.2 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 J331.6034+39.6950 | 22:06:26.14 +39:41:59.3 (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 J331.6034+39.6950,2461120.9494,12.30,0.05,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 J331.6034+39.6950 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:29.39 +39:42:25.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1953651984391739904,2461120.9494,12.21,0.05,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 1953651984391739904 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:27.72 +38:25:55.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.28 21:59:28.75 +37:59:45.7
89.39576 -13.43371 galactic Lac Second-epoch detections are separated by 1.8" and 1.4 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 J329.8746+37.9877 | 21:59:28.75 +37:59:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J329.8746+37.9877,2461120.9494,12.28,0.05,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 J329.8746+37.9877 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:28.75 +37:59:45.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.34 21:49:18.24 +39:21:11.7
88.70968 -11.12375 galactic Cyg Second-epoch detections are separated by 1.5" and 1.3 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 1953373464350864000 | 21:49:16.42 +39:21:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-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
Gaia DR3 1953373464350864000,2461120.9494,12.34,0.05,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 1953373464350864000 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:18.24 +39:21:11.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.25 21:41:04.40 +37:19:14.5
86.10534 -11.58830 galactic Cyg Second-epoch detections are separated by 2.2" and 1.6 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 | Gaia DR3 1952691251747209088 | 21:41:02.35 +37:19:26.6 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.731+/-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
Gaia DR3 1952691251747209088,2461120.9494,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1952691251747209088 20260321.4494 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:04.40 +37:19:14.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.21,0.05,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
target 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:04.07 +39:59:11.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.21 21:50:28.68 +37:17:46.6
87.52702 -12.84010 galactic Cyg Second-epoch detections are separated by 0.5" and 1.3 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 J327.6146+37.2867 | 21:50:28.68 +37:17:46.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.697+/-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 J327.6146+37.2867,2461120.9494,12.21,0.05,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 J327.6146+37.2867 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:28.68 +37:17:46.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.32 21:30:51.99 +34:46:06.8
82.78403 -12.03494 galactic Cyg Second-epoch detections are separated by 0.9" and 1.5 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 J322.7141+34.7705 | 21:30:51.99 +34:46:06.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.439+/-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 J322.7141+34.7705,2461120.9494,12.32,0.05,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 J322.7141+34.7705 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:51.99 +34:46:06.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.35 22:09:33.53 +41:54:58.7
93.40408 -11.48991 galactic Lac Second-epoch detections are separated by 0.6" and 1.3 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 | 22:09:33.53 +41:54:58.7 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.039 (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,2461120.9494,12.35,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:33.53 +41:54:58.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.40 22:02:05.77 +41:42:42.2
92.14509 -10.81941 galactic Lac Second-epoch detections are separated by 1.3" and 1.4 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 J330.5172+41.7159 | 22:02:01.69 +41:42:39.4 (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 J330.5172+41.7159,2461120.9494,12.40,0.05,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 J330.5172+41.7159 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:05.77 +41:42:42.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.24 21:59:01.70 +36:26:59.5
88.32584 -14.58309 galactic Peg Second-epoch detections are separated by 1.0" and 1.3 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 1949636430486534272 | 21:59:02.65 +36:26:18.3 (Gaia DR3) | VAR (local) | F (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1949636430486534272,2461120.9494,12.24,0.05,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
Gaia DR3 1949636430486534272 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:01.70 +36:26:59.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1855196181326170496,2461120.9494,12.18,0.05,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 1855196181326170496 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:29.43 +34:45:43.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1959956068669176064,2461120.9494,12.35,0.05,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 1959956068669176064 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:20.22 +41:45:33.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1953805778581952256,2461120.9494,12.24,0.05,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
Gaia DR3 1953805778581952256 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:26.09 +38:30:21.9 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.37,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:25.42 +36:06:47.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.41 21:48:08.06 +39:26:19.1
88.59090 -10.91217 galactic Cyg Second-epoch detections are separated by 2.2" and 1.0 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 J327.0163+39.4455 | 21:48:06.78 +39:26:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-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 J327.0163+39.4455,2461120.9494,12.41,0.05,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 J327.0163+39.4455 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:08.06 +39:26:19.1 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.29 21:42:24.50 +38:38:04.2
87.19962 -10.78646 galactic Cyg Second-epoch detections are separated by 0.3" and 1.4 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 | 21:42:24.50 +38:38:04.2 (user input) | T | P | (position from user input) J-Ks=0.448+/-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,2461120.9494,12.29,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:24.50 +38:38:04.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.39 21:43:03.31 +37:32:30.8
86.55508 -11.68666 galactic Cyg Second-epoch detections are separated by 1.9" and 1.2 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 | 21:43:03.31 +37:32:30.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461120.9494,12.39,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:03.31 +37:32:30.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.37 22:09:11.53 +36:46:06.5
90.19482 -15.58566 galactic Lac Second-epoch detections are separated by 5.2" 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 J332.2936+36.7689 | 22:09:11.53 +36:46:06.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.423+/-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 J332.2936+36.7689,2461120.9494,12.37,0.05,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 J332.2936+36.7689 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:11.53 +36:46:06.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.21 21:37:55.53 +36:14:19.2
84.88400 -11.96045 galactic Cyg Second-epoch detections are separated by 1.0" and 1.4 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 J324.4847+36.2365 | 21:37:55.53 +36:14:19.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.464+/-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 J324.4847+36.2365,2461120.9494,12.21,0.05,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 J324.4847+36.2365 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:55.53 +36:14:19.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.56 21:38:09.00 +35:14:31.3
84.22364 -12.72152 galactic Cyg Second-epoch detections are separated by 0.9" and 1.4 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 | Large-amplitude variable Gaia DR2 1950725702915116544 | 21:38:09.50 +35:13:51.7 (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 1950725702915116544,2461120.9494,12.56,0.05,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
Large-amplitude variable Gaia DR2 1950725702915116544 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:09.00 +35:14:31.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.31 21:21:10.26 +36:46:15.2
82.81024 -9.22866 galactic Cyg Second-epoch detections are separated by 1.8" and 1.4 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 1963674685717344640 | 21:21:09.19 +36:45:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.045 (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 1963674685717344640,2461120.9494,12.31,0.05,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
Gaia DR3 1963674685717344640 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:10.26 +36:46:15.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.47 22:14:42.67 +40:16:53.2
93.23398 -13.38388 galactic Lac Second-epoch detections are separated by 4.0" and 0.6 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 | Gaia DR3 1957181073116400256 | 22:14:45.40 +40:16:32.6 (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 1957181073116400256,2461120.9494,12.47,0.05,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 1957181073116400256 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:42.67 +40:16:53.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1963882420391944576,2461120.9494,12.32,0.05,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 1963882420391944576 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:39.27 +36:58:21.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.32 21:57:59.38 +41:37:14.4
91.47326 -10.41889 galactic Lac Second-epoch detections are separated by 2.9" and 1.7 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 1959984174936797696 | 21:57:55.98 +41:36:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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
Gaia DR3 1959984174936797696,2461120.9494,12.32,0.05,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 1959984174936797696 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:59.38 +41:37:14.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.47 21:38:09.35 +36:54:29.2
85.38305 -11.50052 galactic Cyg Second-epoch detections are separated by 3.4" and 0.8 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 1951924411105727616 | 21:38:12.46 +36:54:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.567+/- (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 1951924411105727616,2461120.9494,12.47,0.05,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 1951924411105727616 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:09.35 +36:54:29.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.38 22:04:36.75 +38:54:16.0
90.78480 -13.33769 galactic Lac Second-epoch detections are separated by 0.2" and 1.5 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 | Gaia DR3 1955939827569816448 | 22:04:34.49 +38:53:59.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1955939827569816448,2461120.9494,12.38,0.05,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 1955939827569816448 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:36.75 +38:54:16.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.45 21:41:14.37 +36:39:28.2
85.67587 -12.10193 galactic Cyg Second-epoch detections are separated by 1.2" and 1.5 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 J325.3060+36.6500 | 21:41:14.37 +36:39:28.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.3060+36.6500,2461120.9494,12.45,0.05,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 J325.3060+36.6500 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:14.37 +36:39:28.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.71 21:42:34.24 +37:51:57.3
86.70237 -11.38113 galactic Cyg Second-epoch detections are separated by 0.1" and 1.4 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 | 21:42:34.24 +37:51:57.3 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.049 (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,2461120.9494,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260321.4494 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:34.24 +37:51:57.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.51 21:21:48.92 +38:58:05.6
84.48626 -7.78056 galactic Cyg Second-epoch detections are separated by 0.9" and 1.4 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 J320.4533+38.9661 | 21:21:46.33 +38:58:25.0 (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 J320.4533+38.9661,2461120.9494,12.51,0.05,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 J320.4533+38.9661 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:48.92 +38:58:05.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.62 21:46:54.04 +39:15:20.6
88.28528 -10.89546 galactic Cyg Second-epoch detections are separated by 4.0" 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 | target | 21:46:54.04 +39:15:20.6 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.040 (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,2461120.9494,12.62,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:54.04 +39:15:20.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.54 21:56:00.61 +37:10:56.4
88.31977 -13.63370 galactic Cyg Second-epoch detections are separated by 1.3" and 1.3 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 | 21:56:00.61 +37:10:56.4 (user input) | T | P | (position from user input) J-Ks=0.478+/-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
target,2461120.9494,12.54,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:00.61 +37:10:56.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.68 21:20:39.42 +35:23:14.4
81.72980 -10.11783 galactic Cyg Second-epoch detections are separated by 2.9" and 1.7 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 J320.1650+35.3857 | 21:20:39.42 +35:23:14.4 (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 J320.1650+35.3857,2461120.9494,12.68,0.05,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 J320.1650+35.3857 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:39.42 +35:23:14.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.72 21:36:33.98 +38:12:28.3
86.04642 -10.33248 galactic Cyg Second-epoch detections are separated by 3.0" and 0.9 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 1953725303776057984 | 21:36:36.22 +38:11:57.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.475+/-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
Gaia DR3 1953725303776057984,2461120.9494,12.72,0.05,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 1953725303776057984 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:33.98 +38:12:28.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.69 21:36:24.13 +40:56:09.6
87.89738 -8.30568 galactic Cyg Second-epoch detections are separated by 1.4" and 1.6 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 J324.0891+40.9406 | 21:36:24.13 +40:56:09.6 (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 J324.0891+40.9406,2461120.9494,12.69,0.05,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 J324.0891+40.9406 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:24.13 +40:56:09.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.56 21:46:38.60 +37:23:34.7
87.00018 -12.26934 galactic Cyg Second-epoch detections are separated by 1.2" and 1.5 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 | 21:46:38.60 +37:23:34.7 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.043 (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,2461120.9494,12.56,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:38.60 +37:23:34.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1960632160939763456,2461120.9494,12.93,0.05,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 1960632160939763456 20260321.4494 12.93CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:17.52 +42:04:58.0 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.60 21:47:31.21 +37:36:06.6
87.27471 -12.22583 galactic Cyg Second-epoch detections are separated by 3.2" and 1.6 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 | Gaia DR3 1952578414364791680 | 21:47:33.82 +37:35:57.2 (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 1952578414364791680,2461120.9494,12.60,0.05,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
Gaia DR3 1952578414364791680 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:31.21 +37:36:06.6 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.57 21:24:44.54 +39:07:52.7
85.00784 -8.06807 galactic Cyg Second-epoch detections are separated by 7.7" and 1.5 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 J321.1934+39.1218 | 21:24:46.68 +39:07:38.5 (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 J321.1934+39.1218,2461120.9494,12.57,0.05,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 J321.1934+39.1218 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:44.54 +39:07:52.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.90 21:23:35.30 +37:36:36.8
83.75813 -8.98318 galactic Cyg Second-epoch detections are separated by 1.1" and 1.6 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 | 21:23:35.30 +37:36:36.8 (user input) | T | P | (position from user input) J-Ks=0.514+/-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,2461120.9494,12.90,0.05,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 20260321.4494 12.90CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:35.30 +37:36:36.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.89 21:51:39.58 +42:01:59.2
90.80643 -9.35630 galactic Cyg Second-epoch detections are separated by 0.5" and 1.3 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 | 21:51:39.58 +42:01:59.2 (user input) | T | P | (position from user input) J-Ks=0.493+/-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,2461120.9494,12.89,0.05,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 20260321.4494 12.89CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:39.58 +42:01:59.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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 1960368484311351680,2461120.9494,12.92,0.05,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
Gaia DR3 1960368484311351680 20260321.4494 12.92CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:53.03 +41:29:33.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 13.00 21:35:29.49 +39:47:59.8
86.98913 -9.02299 galactic Cyg Second-epoch detections are separated by 2.6" and 1.2 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 | 21:35:29.49 +39:47:59.8 (user input) | T | P | (position from user input) J-Ks=0.525+/-0.040 (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,2461120.9494,13.00,0.05,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
target 20260321.4494 13.00CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:29.49 +39:47:59.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.93 21:23:17.77 +34:21:30.8
81.36282 -11.22297 galactic Cyg Second-epoch detections are separated by 3.3" and 1.9 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 | 21:23:17.77 +34:21:30.8 (user input) | T | P | (position from user input) J-Ks=0.461+/-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,2461120.9494,12.93,0.05,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
target 20260321.4494 12.93CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:17.77 +34:21:30.8 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.99 21:56:43.39 +41:51:09.4
91.43220 -10.09027 galactic Cyg Second-epoch detections are separated by 3.3" and 1.7 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 J329.1700+41.8569 | 21:56:43.39 +41:51:09.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.515+/-0.040 (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 J329.1700+41.8569,2461120.9494,12.99,0.05,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
ATO J329.1700+41.8569 20260321.4494 12.99CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:43.39 +41:51:09.4 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.85 21:23:15.04 +39:36:00.3
85.13620 -7.53262 galactic Cyg Second-epoch detections are separated by 5.3" and 0.7 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 J320.7894+39.5867 | 21:23:11.97 +39:35:40.6 (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 J320.7894+39.5867,2461120.9494,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.7894+39.5867 20260321.4494 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:15.04 +39:36:00.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 13.06 21:52:16.24 +41:27:10.3
90.52078 -9.87626 galactic Cyg Second-epoch detections are separated by 1.0" and 1.2 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 | 21:52:16.24 +41:27:10.3 (user input) | T | P | (position from user input) J-Ks=0.508+/-0.040 (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,2461120.9494,13.06,0.05,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
target 20260321.4494 13.06CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:16.24 +41:27:10.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.91 21:49:05.08 +37:22:34.2
87.36442 -12.59941 galactic Cyg Second-epoch detections are separated by 0.2" and 1.3 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 | 21:49:05.08 +37:22:34.2 (user input) | T | P | (position from user input) J-Ks=0.446+/-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,2461120.9494,12.91,0.05,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
target 20260321.4494 12.91CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:05.08 +37:22:34.2 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.98,0.05,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
target 20260321.4494 12.98CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:54.70 +40:43:52.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 13.01 21:36:32.75 +39:08:53.3
86.69183 -9.63957 galactic Cyg Second-epoch detections are separated by 2.9" and 1.4 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 1953851026054322304 | 21:36:30.57 +39:09:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.412+/-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
Gaia DR3 1953851026054322304,2461120.9494,13.01,0.05,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 1953851026054322304 20260321.4494 13.01CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:32.75 +39:08:53.3 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.77 21:45:18.26 +37:39:35.7
86.97574 -11.89362 galactic Cyg Second-epoch detections are separated by 1.9" and 1.3 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 1952759833784056192 | 21:45:16.89 +37:39:00.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.574+/-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
Gaia DR3 1952759833784056192,2461120.9494,12.77,0.05,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
Gaia DR3 1952759833784056192 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:18.26 +37:39:35.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4494 2461120.9494 12.98 21:50:24.88 +41:23:23.5
90.20831 -9.70244 galactic Cyg Second-epoch detections are separated by 2.5" and 1.5 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 J327.6009+41.3913 | 21:50:24.88 +41:23:23.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.478+/-0.042 (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 J327.6009+41.3913,2461120.9494,12.98,0.05,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 J327.6009+41.3913 20260321.4494 12.98CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:24.88 +41:23:23.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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,2461120.9494,12.81,0.05,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 20260321.4494 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:34.25 +34:35:51.5 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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
IT Peg,2461120.9494,10.65,0.05,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
IT Peg 20260321.4494 10.65CV 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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:42.56 +35:43:46.5 ;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-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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
WW Peg,2461120.9494,10.60,0.05,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
WW Peg 20260321.4494 10.60CV 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:38.07 +36:20:34.7 ;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-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20_00sec_-15_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20_00sec_-15_00C_LIGHT_0486_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: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
First image: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Last image: 2461120.94966797 21.03.2026 10:47:21.313 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 7 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): 24498
Objects passed selection criteria: 24412
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 19888
Average stars matched: 18525.5 (93.1491 %)
Memory usage VmPeak: 128448 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 05:50:46 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: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
First image: 2461032.59720919 23.12.2025 02:19:48.874 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Last image: 2461120.94966797 21.03.2026 10:47:21.313 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 448
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.43
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: 100 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): 180076
Objects passed selection criteria: 179578
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 149717
Average stars matched: 138290 (92.3679 %)
Memory usage VmPeak: 1989520 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 05:53:56 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.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: 2461120.94916341
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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits'
The image scale is 5.78"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:07.345 +37:58:34.65
Angular distance between the image centers 0.08 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 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:08.008 +37:58:33.15
Angular distance between the image centers 0.08 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 21:49:07.345 +37:58:34.65
Second-epoch second image center 21:49:08.008 +37:58:33.15
Angular distance between the image centers 0.00222 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.73HDOnVSXh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.91UxuFsXZT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits &> /tmp/tmp.ZWYdSytrp4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits &> /tmp/tmp.4ScQcco9gr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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 53 out of 28648 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.917418
a=0.000000 b=1.000000 c=22.917418
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
2.2 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.4 pix fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
2.5 pix fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Limiting magnitude estimates:
15.1 mag. Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
15.1 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
14.7 mag. fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
14.7 mag. fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.9 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.73HDOnVSXh (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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2966, passed=28648
Got 28648 stars (including 25648 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 28648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 923.2'
Seting catalog search parameters based on the expected field of view 923.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012822 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010258 (36.9 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 373 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: 4.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.34"
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 467 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.39"
Estimated accuracy of the plate solution: 6.34"
Excluding outliers - 409 stars left (next iteration limit 332)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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.91UxuFsXZT (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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2960, passed=28429
Got 28429 stars (including 25433 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 28429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 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 424 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: 3.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.46"
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 495 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.41"
Estimated accuracy of the plate solution: 2.48"
Excluding outliers - 452 stars left (next iteration limit 410)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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.ZWYdSytrp4 (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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1455, passed=19851
Got 19851 stars (including 18377 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat
util/solve_plate_with_UCAC5 got 19851 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 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: 0.60"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.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.4ScQcco9gr (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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1427, passed=19879
Got 19879 stars (including 18435 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat
util/solve_plate_with_UCAC5 got 19879 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 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 960 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out10857.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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: 1s
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Considering the candidate 31374_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 31374_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:39:52.79 +41:57:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 0.177 1966808809250286976 324.96999208243 +41.96243116639 11.6624 11.2064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 31905_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 31905_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:25:51.54 +36:39:52.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32227_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 32227_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:51:19.36 +36:49:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32254_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 32254_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:48:08.78 +42:09:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 0.412 1960587428864023296 327.03644536495 +42.16642098915 10.7940 10.4802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 32596_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 32596_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:48:31.47 +42:05:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33625_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 33625_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:49:56.76 +40:56:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34004_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 34004_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:24:39.80 +33:48:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 1.098 1855080114127721728 321.16619335315 +33.80592072295 11.7492 10.9477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 34415_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 34415_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:50:15.72 +35:39:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.875 1949260878546849536 327.56564057233 +35.65960337615 11.4772 10.4690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 34795_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 34795_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:24:56.25 +37:11:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.143 1963793261174257152 321.23536600714 +37.18820597676 12.2607 11.8353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 34800_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 34800_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 22:02:33.49 +37:36:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.758 1955703943666369408 330.63977872066 +37.60777044898 12.4561 11.8623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 35091_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 35091_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:49:21.29 +38:22:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.906 1953190666242660352 327.34004141101 +38.37045898839 12.6975 12.1430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 10857_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 10857_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cyg-07-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 ####
22:12:51.18 +39:09:59.3
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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits exists and is non-empty
The image scale is 5.78"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:07.345 +37:58:34.65
Angular distance between the image centers 0.08 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 21:48:48.775 +38:01:54.18
Second-epoch image center 21:49:08.008 +37:58:33.15
Angular distance between the image centers 0.08 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 21:49:07.345 +37:58:34.65
Second-epoch second image center 21:49:08.008 +37:58:33.15
Angular distance between the image centers 0.00222 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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.Z111IJv7w7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.M4TiDlsm4S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits &> /tmp/tmp.cHLL2XlO1B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits &> /tmp/tmp.ONuhHrBeWb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-2 149 out of 201016 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.958293
a=0.000000 b=1.000000 c=20.958293
From vast_summary.log: estimated ref. image limiting mag.: -7.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.53
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 358 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
2.1 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.3 pix fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
2.3 pix fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Limiting magnitude estimates:
13.5 mag. Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
13.5 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
13.0 mag. fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
13.0 mag. fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.4 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Z111IJv7w7 (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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=28576, passed=200971
Got 200971 stars (including 172048 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 200971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 923.2'
Seting catalog search parameters based on the expected field of view 923.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012822 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010258 (36.9 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 369 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: 4.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.09"
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 467 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.09"
Estimated accuracy of the plate solution: 5.74"
Excluding outliers - 413 stars left (next iteration limit 325)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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.M4TiDlsm4S (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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=65, blended=28738, passed=202040
Got 202040 stars (including 172959 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 202040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 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 409 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: 3.16"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.60"
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 485 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.59"
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 456 stars left (next iteration limit 405)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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.cHLL2XlO1B (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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=16239, passed=141285
Got 141285 stars (including 124891 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat
util/solve_plate_with_UCAC5 got 141285 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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: 0.54"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.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.ONuhHrBeWb (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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=16174, passed=141543
Got 141543 stars (including 125200 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat
util/solve_plate_with_UCAC5 got 141543 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 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 963 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: 0.60"
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 963 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: 0.60"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.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-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits
Saving fully-calibrated image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-46-37_20.00sec_-15.00C_LIGHT_0486.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.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_2026-03-21_CI_Cyg-07-Q2b1x1_054829_TTUQ2b1x1_10880_QqX99JtN/wcs_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487.fits
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out245079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out252334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out138402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227019.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out227037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227054.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out253085.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 287s
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: 140s
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Considering the candidate 226854_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226854_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226855_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226855_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226856_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226856_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226859_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226859_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226866_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226866_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226868_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226868_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226872_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226872_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226887_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226887_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226891_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226891_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226893_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226893_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226894_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226894_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226906_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226906_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226922_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226922_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226923_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226923_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226928_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226928_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226934_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 226934_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226936_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226936_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226937_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226937_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226938_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226938_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226943_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226943_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226946_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226946_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226948_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226948_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226952_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226952_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226959_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226959_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226965_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226965_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226967_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226967_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226968_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226968_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226971_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226971_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226972_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 226972_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226981_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226981_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226982_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226982_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226987_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226987_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226988_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226988_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226993_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226993_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226995_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226995_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226996_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226996_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 226998_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 226998_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227001_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227001_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227002_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227002_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227003_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227003_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227004_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227004_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227007_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227007_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227010_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227010_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227011_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227011_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227014_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227014_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227017_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227017_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227019_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227019_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227024_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227024_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227025_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227025_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227028_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227028_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227029_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227029_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227037_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227037_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227043_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227043_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227048_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227048_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227053_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 227053_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 227054_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227054_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227058_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227058_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227059_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227059_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227060_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227060_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227062_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227062_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227063_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227063_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227065_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227065_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227070_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227070_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227075_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227075_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227078_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227078_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227079_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227079_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227080_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227080_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227085_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227085_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227091_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 227091_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 227609_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 227609_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:25:51.32 +36:39:54.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 229013_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 229013_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 229964_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 229964_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 230390_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 230390_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 230779_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 230779_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 231508_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 231508_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 231979_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 231979_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 232113_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 232113_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 232187_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 232187_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 232743_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 232743_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 232905_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 232905_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 232947_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 232947_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 233118_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 233118_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 233215_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 233215_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234010_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 234010_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234044_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 234044_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234065_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 234065_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 234284_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 234284_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 234422_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 234422_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 234450_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 234450_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234858_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 234858_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235024_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235024_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235028_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235028_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235034_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 235034_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 235133_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235133_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235167_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235167_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235176_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 235176_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 235304_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235304_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235383_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 235383_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 235409_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 235409_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 235492_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235492_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235549_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 235549_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 235568_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235568_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235657_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 235657_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 235832_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 235832_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236044_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 236044_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 236092_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 236092_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 236202_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 236202_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236328_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 236328_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236404_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 236404_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:48:22.57 +38:39:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236462_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 236462_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236582_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 236582_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 236672_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 236672_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236768_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 236768_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236978_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 236978_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 236985_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 236985_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237021_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 237021_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237107_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 237107_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237203_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 237203_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237311_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 237311_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 237364_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 237364_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 237426_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 237426_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 237606_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 237606_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 237821_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 237821_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 237844_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 237844_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 237937_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 237937_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 238125_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 238125_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 238281_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 238281_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 238377_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 238377_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 238606_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 238606_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 238676_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 238676_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 238707_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 238707_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 238717_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 238717_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:20:13.93 +37:24:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 238770_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 238770_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239145_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 239145_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 239162_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 239162_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239183_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 239183_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 239209_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 239209_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 239222_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 239222_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 239234_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 239234_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239275_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 239275_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:51:45.89 +41:39:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239288_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 239288_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239327_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 239327_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239472_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 239472_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239485_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 239485_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239775_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 239775_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 239839_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 239839_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 240094_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 240094_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 240150_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 240150_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 240751_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 240751_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 240785_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 240785_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 240803_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 240803_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 240826_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 240826_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 240895_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 240895_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 240986_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 240986_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241026_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 241026_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 241144_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 241144_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:23:27.94 +37:25:55.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 241148_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241148_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241307_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 241307_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 241422_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241422_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241491_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241491_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241507_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 241507_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 241573_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241573_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241699_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241699_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241850_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241850_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241859_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241859_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241890_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241890_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241919_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 241919_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 241938_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241938_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241940_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241940_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 241951_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 241951_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242040_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 242040_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 242163_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242163_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242194_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242194_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242261_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242261_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242264_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242264_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242350_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242350_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242441_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 242441_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:47:58.36 +36:34:46.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242447_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242447_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242454_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 242454_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 242532_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242532_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242619_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 242619_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 242641_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242641_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242646_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 242646_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 242721_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 242721_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 242759_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242759_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242773_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242773_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242781_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242781_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 242973_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 242973_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243130_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243130_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243201_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243201_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243360_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243360_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243366_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 243366_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 243368_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243368_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243390_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 243390_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 243419_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243419_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243648_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243648_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243651_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243651_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243661_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243661_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243798_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243798_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243895_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243895_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243932_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243932_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243954_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243954_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 243969_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 243969_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244077_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244077_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244102_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 244102_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 244133_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244133_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244392_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244392_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244518_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244518_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244568_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244568_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244596_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 244596_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 244746_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244746_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244749_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244749_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244755_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244755_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244809_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244809_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244821_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244821_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244867_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244867_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 244883_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 244883_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245020_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245020_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245079_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245079_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:51:29.42 +38:43:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.857 1953105905067981952 327.87158794961 +38.71955905257 11.8663 9.9472 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 245116_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245116_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245208_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245208_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 245219_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245219_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 245256_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245256_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 245317_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245317_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245331_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245331_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245345_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245345_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 245360_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245360_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 245371_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245371_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 245439_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245439_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245490_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245490_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245510_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245510_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245550_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245550_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245631_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245631_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245704_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245704_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245735_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245735_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 245853_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245853_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245893_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245893_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 245904_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 245904_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 245960_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 245960_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246102_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246102_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246134_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246134_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246157_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 246157_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 246169_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 246169_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 246273_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 246273_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 246312_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 246312_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 246340_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246340_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246369_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246369_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246404_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246404_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246420_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246420_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246523_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246523_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246552_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 246552_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 246608_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246608_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246620_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246620_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246713_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 246713_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 246760_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 246760_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 246769_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246769_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246796_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246796_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246820_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246820_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 246864_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 246864_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 247204_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 247204_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 247265_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 247265_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247301_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 247301_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247391_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 247391_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 247446_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 247446_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 247449_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 247449_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 247523_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 247523_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 247748_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 247748_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247944_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 247944_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 248001_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248001_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248008_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248008_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248064_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 248064_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 248291_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 248291_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 248309_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248309_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248328_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248328_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248339_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248339_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248360_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 248360_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 248405_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 248405_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 248446_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248446_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248448_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 248448_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 248611_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 248611_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 248651_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248651_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248710_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248710_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 248830_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 248830_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 249004_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 249004_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 249043_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 249043_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 249081_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 249081_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 249276_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 249276_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 249622_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 249622_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 249637_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 249637_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 249639_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 249639_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 249847_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 249847_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 249947_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 249947_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 250054_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 250054_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 250124_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 250124_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 250137_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 250137_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 250305_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 250305_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 250365_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 250365_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 250444_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 250444_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 250664_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 250664_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 250671_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 250671_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 250707_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 250707_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 250812_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 250812_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 250883_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 250883_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 250975_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 250975_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 251018_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251018_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251046_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251046_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251052_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 251052_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 251110_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 251110_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 251196_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251196_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251233_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251233_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 251326_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251326_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251336_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 251336_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 251375_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251375_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251473_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251473_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251485_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251485_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251659_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 251659_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 251829_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 251829_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 251995_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 251995_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 251997_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 251997_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252068_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252068_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252251_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252251_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252334_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252334_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:21:27.78 +37:08:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.680 1963899707643448448 320.36580516621 +37.13649250162 13.4013 12.0717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 252346_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252346_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 252394_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252394_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 252411_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252411_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252445_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252445_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252465_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252465_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252466_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252466_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 252577_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252577_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252619_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252619_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252630_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252630_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252658_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252658_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252757_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252757_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252796_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252796_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252809_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252809_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252815_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252815_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252823_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252823_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252830_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252830_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252845_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252845_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252870_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 252870_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 252942_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252942_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252995_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252995_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 252996_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 252996_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 253051_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 253051_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 253085_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 253085_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 113380_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 113380_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219051_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 219051_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 76443_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 76443_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 22:12:51.18 +39:09:59.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 47611_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 47611_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:49:56.79 +40:56:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129504_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 129504_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:51:19.38 +36:49:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106787_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 106787_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224067_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 224067_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138402_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
Preparing report for the candidate 138402_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
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Considering the candidate 221197_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 221197_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 97159_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 97159_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 23941_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 23941_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 24612_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 24612_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
**** FOUND 21:48:31.49 +42:05:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25448_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487
The candidate 25448_fd_Cyg-07-Q2b1x1_2026-03-21_05-47-21_20.00sec_-15.00C_LIGHT_0487 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
make_report_in_HTML.sh Phase 2 (HTML assembly): 58s
make_report_in_HTML.sh TOTAL: 485s
Prepared the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:12:51.18 +39:09:59.3
21:56:38.07 +36:20:34.7
22:03:42.56 +35:43:46.5
21:34:15.55 +38:14:21.3
21:32:46.01 +37:06:20.5
21:45:43.36 +41:42:23.0
21:24:50.19 +39:27:06.1
21:41:45.14 +37:40:54.2
21:27:24.07 +36:58:25.0
21:49:38.29 +41:30:55.0
21:31:35.18 +38:09:23.1
21:21:46.40 +35:01:45.8
21:30:47.82 +38:57:32.5
21:23:31.33 +39:22:16.0
21:44:37.38 +38:02:19.2
21:44:52.81 +37:32:27.1
21:20:08.98 +38:06:51.3
21:28:02.73 +38:25:44.9
21:22:16.36 +36:13:44.9
21:56:58.95 +36:20:20.9
22:02:54.19 +40:52:41.4
21:39:13.08 +42:06:32.0
21:50:55.94 +34:03:39.1
21:47:50.79 +40:31:46.2
21:34:26.75 +41:42:34.0
21:47:52.58 +34:30:12.8
21:43:05.23 +41:29:28.1
21:22:46.56 +34:59:22.5
21:53:53.73 +41:17:51.7
21:40:12.85 +36:18:00.6
22:15:11.65 +39:02:25.1
21:41:28.51 +41:30:43.6
21:27:41.77 +38:45:45.4
21:19:17.68 +37:56:05.4
21:44:39.07 +41:53:49.7
21:57:22.83 +40:56:51.4
21:22:31.09 +37:35:51.7
21:48:18.10 +41:54:23.7
22:03:59.00 +40:08:16.2
21:45:28.84 +42:12:24.4
21:20:00.19 +38:24:37.2
21:38:44.95 +35:57:35.2
21:23:57.85 +34:02:50.2
21:25:35.29 +34:11:53.2
21:22:57.47 +38:21:11.6
21:31:14.96 +36:19:50.3
21:31:29.29 +40:58:23.7
21:45:53.74 +35:13:19.2
21:20:31.14 +38:20:14.1
21:20:26.99 +35:31:37.1
21:32:48.46 +39:29:41.6
21:58:37.13 +33:56:11.7
21:19:18.67 +37:19:00.9
21:18:47.35 +38:10:22.2
21:26:04.93 +37:38:02.0
21:22:26.13 +37:11:04.3
21:19:57.19 +39:52:25.7
22:00:14.39 +41:40:34.0
21:55:20.92 +40:52:13.1
22:13:41.76 +40:56:39.1
21:28:47.08 +42:05:19.1
21:51:52.25 +41:19:33.8
21:18:16.76 +37:55:32.6
21:28:09.28 +41:14:36.0
21:18:26.49 +38:35:23.1
21:54:25.00 +39:39:27.7
21:46:27.10 +42:00:03.0
21:31:37.92 +34:11:28.6
21:23:53.58 +35:33:45.7
21:24:39.85 +33:48:21.5
21:39:25.90 +41:43:13.8
21:47:57.33 +36:35:33.9
21:31:14.81 +39:26:58.6
21:42:55.14 +41:10:20.0
21:42:50.27 +37:29:32.7
21:27:46.08 +35:33:54.1
21:35:04.78 +40:51:23.3
22:08:33.83 +41:26:35.6
21:52:09.56 +38:58:10.1
21:58:48.44 +41:41:43.3
21:39:05.39 +36:51:24.2
22:13:14.65 +41:47:42.9
21:56:37.89 +37:20:32.3
21:33:36.34 +38:32:50.2
22:12:58.64 +38:26:20.3
21:18:40.03 +39:14:36.1
21:41:29.15 +37:46:45.6
21:32:54.35 +35:30:10.4
21:20:46.72 +33:50:41.5
21:39:07.89 +36:52:27.7
22:07:50.36 +40:07:28.2
21:48:53.62 +40:38:12.4
21:19:36.10 +38:11:41.1
21:35:30.51 +34:46:53.2
21:22:57.16 +34:21:06.6
21:55:05.31 +34:46:30.7
21:58:07.76 +38:56:42.0
22:01:49.89 +36:55:26.7
22:06:46.19 +39:39:09.6
21:42:50.12 +38:10:45.9
21:42:06.19 +36:50:53.8
22:11:23.05 +39:44:15.2
21:26:53.38 +34:58:18.2
22:13:05.31 +41:48:40.8
22:00:54.57 +41:16:15.2
21:42:21.28 +34:05:46.6
21:39:20.65 +35:38:18.7
21:44:49.77 +36:56:55.7
21:49:54.58 +34:54:44.0
21:50:52.30 +39:37:43.0
22:04:00.09 +39:46:41.1
22:21:21.26 +41:17:36.3
21:23:19.64 +35:13:30.0
22:16:38.13 +41:45:37.6
22:02:40.25 +38:06:45.2
21:59:02.61 +37:17:54.7
22:13:03.63 +38:28:17.9
21:39:39.54 +39:57:28.3
21:21:16.92 +34:59:15.3
21:57:20.62 +40:57:00.4
22:06:31.79 +34:33:33.0
21:27:05.58 +36:00:32.0
21:20:36.26 +35:29:43.0
21:36:04.29 +41:56:44.6
21:54:04.37 +37:39:41.1
21:52:31.17 +41:28:58.3
21:43:16.93 +40:27:46.9
21:35:06.90 +38:39:19.6
22:02:27.76 +42:04:01.6
21:18:30.05 +39:08:10.7
21:50:11.57 +35:33:08.5
21:38:09.28 +38:56:17.1
22:09:46.26 +41:39:58.4
21:27:48.41 +38:33:03.8
21:46:21.76 +39:50:08.5
21:49:12.20 +34:20:08.5
21:21:51.04 +37:53:26.0
21:41:09.87 +36:39:08.8
21:43:32.06 +38:44:15.1
21:43:30.47 +41:30:12.3
21:22:07.84 +36:03:45.4
21:49:54.43 +37:45:56.6
21:34:12.43 +39:03:18.4
21:57:34.03 +41:27:52.3
21:39:00.67 +38:41:34.2
21:26:29.31 +39:08:36.1
22:05:11.32 +39:28:34.7
21:58:43.28 +42:11:58.3
22:05:42.75 +35:53:01.3
21:51:54.98 +33:54:39.2
21:56:45.17 +36:22:45.2
21:32:57.30 +38:12:17.6
21:36:34.05 +37:11:49.1
22:13:03.64 +38:27:56.2
21:40:39.17 +41:35:37.9
21:29:19.08 +40:28:36.3
22:10:19.95 +38:44:17.5
21:31:28.76 +34:33:30.8
22:15:17.59 +39:47:56.7
21:23:16.30 +35:12:48.0
21:30:29.32 +34:39:52.2
21:58:13.58 +38:26:16.0
21:36:06.03 +34:59:43.1
22:00:00.17 +38:42:22.9
21:46:36.46 +37:39:35.6
21:36:02.24 +39:50:06.7
21:25:10.35 +36:09:27.9
22:18:15.73 +40:51:52.2
21:38:38.15 +33:58:30.9
21:57:15.92 +39:56:53.4
21:58:15.48 +41:40:34.6
21:40:29.72 +38:25:54.2
22:06:29.39 +39:42:25.0
21:40:27.72 +38:25:55.7
21:59:28.75 +37:59:45.7
21:49:18.24 +39:21:11.7
21:41:04.40 +37:19:14.5
22:06:04.07 +39:59:11.7
21:50:28.68 +37:17:46.6
21:30:51.99 +34:46:06.8
22:09:33.53 +41:54:58.7
22:02:05.77 +41:42:42.2
21:59:01.70 +36:26:59.5
21:25:29.43 +34:45:43.1
22:01:20.22 +41:45:33.5
21:34:26.09 +38:30:21.9
21:28:25.42 +36:06:47.3
21:48:08.06 +39:26:19.1
21:42:24.50 +38:38:04.2
21:43:03.31 +37:32:30.8
22:09:11.53 +36:46:06.5
21:37:55.53 +36:14:19.2
21:38:09.00 +35:14:31.3
21:21:10.26 +36:46:15.2
22:14:42.67 +40:16:53.2
21:19:39.27 +36:58:21.7
21:57:59.38 +41:37:14.4
21:38:09.35 +36:54:29.2
22:04:36.75 +38:54:16.0
21:41:14.37 +36:39:28.2
21:42:34.24 +37:51:57.3
21:21:48.92 +38:58:05.6
21:46:54.04 +39:15:20.6
21:56:00.61 +37:10:56.4
21:20:39.42 +35:23:14.4
21:36:33.98 +38:12:28.3
21:36:24.13 +40:56:09.6
21:46:38.60 +37:23:34.7
21:50:17.52 +42:04:58.0
21:47:31.21 +37:36:06.6
21:24:44.54 +39:07:52.7
21:23:35.30 +37:36:36.8
21:51:39.58 +42:01:59.2
21:54:53.03 +41:29:33.8
21:35:29.49 +39:47:59.8
21:23:17.77 +34:21:30.8
21:56:43.39 +41:51:09.4
21:23:15.04 +39:36:00.3
21:52:16.24 +41:27:10.3
21:49:05.08 +37:22:34.2
21:42:54.70 +40:43:52.5
21:36:32.75 +39:08:53.3
21:45:18.26 +37:39:35.7
21:50:24.88 +41:23:23.5
21:35:34.25 +34:35:51.5
########### Completed Cyg-07-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 ####
22:12:51.18 +39:09:59.3
21:34:15.55 +38:14:21.3
21:32:46.01 +37:06:20.5
21:45:43.36 +41:42:23.0
21:24:50.19 +39:27:06.1
21:41:45.14 +37:40:54.2
21:27:24.07 +36:58:25.0
21:49:38.29 +41:30:55.0
21:31:35.18 +38:09:23.1
21:21:46.40 +35:01:45.8
21:30:47.82 +38:57:32.5
21:23:31.33 +39:22:16.0
21:44:37.38 +38:02:19.2
21:44:52.81 +37:32:27.1
21:20:08.98 +38:06:51.3
21:28:02.73 +38:25:44.9
21:22:16.36 +36:13:44.9
21:56:58.95 +36:20:20.9
22:02:54.19 +40:52:41.4
21:39:13.08 +42:06:32.0
21:50:55.94 +34:03:39.1
21:47:50.79 +40:31:46.2
21:34:26.75 +41:42:34.0
21:47:52.58 +34:30:12.8
21:43:05.23 +41:29:28.1
21:22:46.56 +34:59:22.5
21:53:53.73 +41:17:51.7
21:40:12.85 +36:18:00.6
22:15:11.65 +39:02:25.1
21:41:28.51 +41:30:43.6
21:27:41.77 +38:45:45.4
21:19:17.68 +37:56:05.4
21:44:39.07 +41:53:49.7
21:57:22.83 +40:56:51.4
21:22:31.09 +37:35:51.7
21:48:18.10 +41:54:23.7
22:03:59.00 +40:08:16.2
21:45:28.84 +42:12:24.4
21:20:00.19 +38:24:37.2
21:38:44.95 +35:57:35.2
21:23:57.85 +34:02:50.2
21:25:35.29 +34:11:53.2
21:22:57.47 +38:21:11.6
21:31:14.96 +36:19:50.3
21:31:29.29 +40:58:23.7
21:45:53.74 +35:13:19.2
21:20:31.14 +38:20:14.1
21:20:26.99 +35:31:37.1
21:32:48.46 +39:29:41.6
21:58:37.13 +33:56:11.7
21:19:18.67 +37:19:00.9
21:18:47.35 +38:10:22.2
21:26:04.93 +37:38:02.0
21:22:26.13 +37:11:04.3
21:19:57.19 +39:52:25.7
22:00:14.39 +41:40:34.0
21:55:20.92 +40:52:13.1
22:13:41.76 +40:56:39.1
21:28:47.08 +42:05:19.1
21:51:52.25 +41:19:33.8
21:18:16.76 +37:55:32.6
21:28:09.28 +41:14:36.0
21:18:26.49 +38:35:23.1
21:54:25.00 +39:39:27.7
21:46:27.10 +42:00:03.0
21:31:37.92 +34:11:28.6
21:23:53.58 +35:33:45.7
21:24:39.85 +33:48:21.5
21:39:25.90 +41:43:13.8
21:47:57.33 +36:35:33.9
21:31:14.81 +39:26:58.6
21:42:55.14 +41:10:20.0
21:42:50.27 +37:29:32.7
21:27:46.08 +35:33:54.1
21:35:04.78 +40:51:23.3
22:08:33.83 +41:26:35.6
21:52:09.56 +38:58:10.1
21:58:48.44 +41:41:43.3
21:39:05.39 +36:51:24.2
22:13:14.65 +41:47:42.9
21:56:37.89 +37:20:32.3
21:33:36.34 +38:32:50.2
22:12:58.64 +38:26:20.3
21:18:40.03 +39:14:36.1
21:41:29.15 +37:46:45.6
21:32:54.35 +35:30:10.4
21:20:46.72 +33:50:41.5
21:39:07.89 +36:52:27.7
22:07:50.36 +40:07:28.2
21:48:53.62 +40:38:12.4
21:19:36.10 +38:11:41.1
21:35:30.51 +34:46:53.2
21:22:57.16 +34:21:06.6
21:55:05.31 +34:46:30.7
21:58:07.76 +38:56:42.0
22:01:49.89 +36:55:26.7
22:06:46.19 +39:39:09.6
21:42:50.12 +38:10:45.9
21:42:06.19 +36:50:53.8
22:11:23.05 +39:44:15.2
21:26:53.38 +34:58:18.2
22:13:05.31 +41:48:40.8
22:00:54.57 +41:16:15.2
21:42:21.28 +34:05:46.6
21:39:20.65 +35:38:18.7
21:44:49.77 +36:56:55.7
21:49:54.58 +34:54:44.0
21:50:52.30 +39:37:43.0
22:04:00.09 +39:46:41.1
22:21:21.26 +41:17:36.3
21:23:19.64 +35:13:30.0
22:16:38.13 +41:45:37.6
22:02:40.25 +38:06:45.2
21:59:02.61 +37:17:54.7
22:13:03.63 +38:28:17.9
21:39:39.54 +39:57:28.3
21:21:16.92 +34:59:15.3
21:57:20.62 +40:57:00.4
22:06:31.79 +34:33:33.0
21:27:05.58 +36:00:32.0
21:20:36.26 +35:29:43.0
21:36:04.29 +41:56:44.6
21:54:04.37 +37:39:41.1
21:52:31.17 +41:28:58.3
21:43:16.93 +40:27:46.9
21:35:06.90 +38:39:19.6
22:02:27.76 +42:04:01.6
21:18:30.05 +39:08:10.7
21:50:11.57 +35:33:08.5
21:38:09.28 +38:56:17.1
22:09:46.26 +41:39:58.4
21:27:48.41 +38:33:03.8
21:46:21.76 +39:50:08.5
21:49:12.20 +34:20:08.5
21:21:51.04 +37:53:26.0
21:41:09.87 +36:39:08.8
21:43:32.06 +38:44:15.1
21:43:30.47 +41:30:12.3
21:22:07.84 +36:03:45.4
21:49:54.43 +37:45:56.6
21:34:12.43 +39:03:18.4
21:57:34.03 +41:27:52.3
21:39:00.67 +38:41:34.2
21:26:29.31 +39:08:36.1
22:05:11.32 +39:28:34.7
21:58:43.28 +42:11:58.3
22:05:42.75 +35:53:01.3
21:51:54.98 +33:54:39.2
21:56:45.17 +36:22:45.2
21:32:57.30 +38:12:17.6
21:36:34.05 +37:11:49.1
22:13:03.64 +38:27:56.2
21:40:39.17 +41:35:37.9
21:29:19.08 +40:28:36.3
22:10:19.95 +38:44:17.5
21:31:28.76 +34:33:30.8
22:15:17.59 +39:47:56.7
21:23:16.30 +35:12:48.0
21:30:29.32 +34:39:52.2
21:58:13.58 +38:26:16.0
21:36:06.03 +34:59:43.1
22:00:00.17 +38:42:22.9
21:46:36.46 +37:39:35.6
21:36:02.24 +39:50:06.7
21:25:10.35 +36:09:27.9
22:18:15.73 +40:51:52.2
21:38:38.15 +33:58:30.9
21:57:15.92 +39:56:53.4
21:58:15.48 +41:40:34.6
21:40:29.72 +38:25:54.2
22:06:29.39 +39:42:25.0
21:40:27.72 +38:25:55.7
21:59:28.75 +37:59:45.7
21:49:18.24 +39:21:11.7
21:41:04.40 +37:19:14.5
22:06:04.07 +39:59:11.7
21:50:28.68 +37:17:46.6
21:30:51.99 +34:46:06.8
22:09:33.53 +41:54:58.7
22:02:05.77 +41:42:42.2
21:59:01.70 +36:26:59.5
21:25:29.43 +34:45:43.1
22:01:20.22 +41:45:33.5
21:34:26.09 +38:30:21.9
21:28:25.42 +36:06:47.3
21:48:08.06 +39:26:19.1
21:42:24.50 +38:38:04.2
21:43:03.31 +37:32:30.8
22:09:11.53 +36:46:06.5
21:37:55.53 +36:14:19.2
21:38:09.00 +35:14:31.3
21:21:10.26 +36:46:15.2
22:14:42.67 +40:16:53.2
21:19:39.27 +36:58:21.7
21:57:59.38 +41:37:14.4
21:38:09.35 +36:54:29.2
22:04:36.75 +38:54:16.0
21:41:14.37 +36:39:28.2
21:42:34.24 +37:51:57.3
21:21:48.92 +38:58:05.6
21:46:54.04 +39:15:20.6
21:56:00.61 +37:10:56.4
21:20:39.42 +35:23:14.4
21:36:33.98 +38:12:28.3
21:36:24.13 +40:56:09.6
21:46:38.60 +37:23:34.7
21:50:17.52 +42:04:58.0
21:47:31.21 +37:36:06.6
21:24:44.54 +39:07:52.7
21:23:35.30 +37:36:36.8
21:51:39.58 +42:01:59.2
21:54:53.03 +41:29:33.8
21:35:29.49 +39:47:59.8
21:23:17.77 +34:21:30.8
21:56:43.39 +41:51:09.4
21:23:15.04 +39:36:00.3
21:52:16.24 +41:27:10.3
21:49:05.08 +37:22:34.2
21:42:54.70 +40:43:52.5
21:36:32.75 +39:08:53.3
21:45:18.26 +37:39:35.7
21:50:24.88 +41:23:23.5
21:35:34.25 +34:35:51.5
22:03:42.56 +35:43:46.5
21:56:38.07 +36:20:34.7
###################################################################################
22:12:51.18 +39:09:59.3 -- not an asteroid (will add it to exclusion list)
21:34:15.55 +38:14:21.3 -- not an asteroid (will add it to exclusion list)
21:32:46.01 +37:06:20.5 -- not an asteroid (will add it to exclusion list)
21:45:43.36 +41:42:23.0 -- not an asteroid (will add it to exclusion list)
21:24:50.19 +39:27:06.1 -- not an asteroid (will add it to exclusion list)
21:41:45.14 +37:40:54.2 -- not an asteroid (will add it to exclusion list)
21:27:24.07 +36:58:25.0 -- not an asteroid (will add it to exclusion list)
21:49:38.29 +41:30:55.0 -- not an asteroid (will add it to exclusion list)
21:31:35.18 +38:09:23.1 -- not an asteroid (will add it to exclusion list)
21:21:46.40 +35:01:45.8 -- not an asteroid (will add it to exclusion list)
21:30:47.82 +38:57:32.5 -- not an asteroid (will add it to exclusion list)
21:23:31.33 +39:22:16.0 -- not an asteroid (will add it to exclusion list)
21:44:37.38 +38:02:19.2 -- not an asteroid (will add it to exclusion list)
21:44:52.81 +37:32:27.1 -- not an asteroid (will add it to exclusion list)
21:20:08.98 +38:06:51.3 -- not an asteroid (will add it to exclusion list)
21:28:02.73 +38:25:44.9 -- not an asteroid (will add it to exclusion list)
21:22:16.36 +36:13:44.9 -- not an asteroid (will add it to exclusion list)
21:56:58.95 +36:20:20.9 -- not an asteroid (will add it to exclusion list)
22:02:54.19 +40:52:41.4 -- not an asteroid (will add it to exclusion list)
21:39:13.08 +42:06:32.0 -- not an asteroid (will add it to exclusion list)
21:50:55.94 +34:03:39.1 -- not an asteroid (will add it to exclusion list)
21:47:50.79 +40:31:46.2 -- not an asteroid (will add it to exclusion list)
21:34:26.75 +41:42:34.0 -- not an asteroid (will add it to exclusion list)
21:47:52.58 +34:30:12.8 -- not an asteroid (will add it to exclusion list)
21:43:05.23 +41:29:28.1 -- not an asteroid (will add it to exclusion list)
21:22:46.56 +34:59:22.5 -- not an asteroid (will add it to exclusion list)
21:53:53.73 +41:17:51.7 -- not an asteroid (will add it to exclusion list)
21:40:12.85 +36:18:00.6 -- not an asteroid (will add it to exclusion list)
22:15:11.65 +39:02:25.1 -- not an asteroid (will add it to exclusion list)
21:41:28.51 +41:30:43.6 -- not an asteroid (will add it to exclusion list)
21:27:41.77 +38:45:45.4 -- not an asteroid (will add it to exclusion list)
21:19:17.68 +37:56:05.4 -- not an asteroid (will add it to exclusion list)
21:44:39.07 +41:53:49.7 -- not an asteroid (will add it to exclusion list)
21:57:22.83 +40:56:51.4 -- not an asteroid (will add it to exclusion list)
21:22:31.09 +37:35:51.7 -- not an asteroid (will add it to exclusion list)
21:48:18.10 +41:54:23.7 -- not an asteroid (will add it to exclusion list)
22:03:59.00 +40:08:16.2 -- not an asteroid (will add it to exclusion list)
21:45:28.84 +42:12:24.4 -- not an asteroid (will add it to exclusion list)
21:20:00.19 +38:24:37.2 -- not an asteroid (will add it to exclusion list)
21:38:44.95 +35:57:35.2 -- not an asteroid (will add it to exclusion list)
21:23:57.85 +34:02:50.2 -- not an asteroid (will add it to exclusion list)
21:25:35.29 +34:11:53.2 -- not an asteroid (will add it to exclusion list)
21:22:57.47 +38:21:11.6 -- not an asteroid (will add it to exclusion list)
21:31:14.96 +36:19:50.3 -- not an asteroid (will add it to exclusion list)
21:31:29.29 +40:58:23.7 -- not an asteroid (will add it to exclusion list)
21:45:53.74 +35:13:19.2 -- not an asteroid (will add it to exclusion list)
21:20:31.14 +38:20:14.1 -- not an asteroid (will add it to exclusion list)
21:20:26.99 +35:31:37.1 -- not an asteroid (will add it to exclusion list)
21:32:48.46 +39:29:41.6 -- not an asteroid (will add it to exclusion list)
21:58:37.13 +33:56:11.7 -- not an asteroid (will add it to exclusion list)
21:19:18.67 +37:19:00.9 -- not an asteroid (will add it to exclusion list)
21:18:47.35 +38:10:22.2 -- not an asteroid (will add it to exclusion list)
21:26:04.93 +37:38:02.0 -- not an asteroid (will add it to exclusion list)
21:22:26.13 +37:11:04.3 -- not an asteroid (will add it to exclusion list)
21:19:57.19 +39:52:25.7 -- not an asteroid (will add it to exclusion list)
22:00:14.39 +41:40:34.0 -- not an asteroid (will add it to exclusion list)
21:55:20.92 +40:52:13.1 -- not an asteroid (will add it to exclusion list)
22:13:41.76 +40:56:39.1 -- not an asteroid (will add it to exclusion list)
21:28:47.08 +42:05:19.1 -- not an asteroid (will add it to exclusion list)
21:51:52.25 +41:19:33.8 -- not an asteroid (will add it to exclusion list)
21:18:16.76 +37:55:32.6 -- not an asteroid (will add it to exclusion list)
21:28:09.28 +41:14:36.0 -- not an asteroid (will add it to exclusion list)
21:18:26.49 +38:35:23.1 -- not an asteroid (will add it to exclusion list)
21:54:25.00 +39:39:27.7 -- not an asteroid (will add it to exclusion list)
21:46:27.10 +42:00:03.0 -- not an asteroid (will add it to exclusion list)
21:31:37.92 +34:11:28.6 -- not an asteroid (will add it to exclusion list)
21:23:53.58 +35:33:45.7 -- not an asteroid (will add it to exclusion list)
21:24:39.85 +33:48:21.5 -- not an asteroid (will add it to exclusion list)
21:39:25.90 +41:43:13.8 -- not an asteroid (will add it to exclusion list)
21:47:57.33 +36:35:33.9 -- not an asteroid (will add it to exclusion list)
21:31:14.81 +39:26:58.6 -- not an asteroid (will add it to exclusion list)
21:42:55.14 +41:10:20.0 -- not an asteroid (will add it to exclusion list)
21:42:50.27 +37:29:32.7 -- not an asteroid (will add it to exclusion list)
21:27:46.08 +35:33:54.1 -- not an asteroid (will add it to exclusion list)
21:35:04.78 +40:51:23.3 -- not an asteroid (will add it to exclusion list)
22:08:33.83 +41:26:35.6 -- not an asteroid (will add it to exclusion list)
21:52:09.56 +38:58:10.1 -- not an asteroid (will add it to exclusion list)
21:58:48.44 +41:41:43.3 -- not an asteroid (will add it to exclusion list)
21:39:05.39 +36:51:24.2 -- not an asteroid (will add it to exclusion list)
22:13:14.65 +41:47:42.9 -- not an asteroid (will add it to exclusion list)
21:56:37.89 +37:20:32.3 -- not an asteroid (will add it to exclusion list)
21:33:36.34 +38:32:50.2 -- not an asteroid (will add it to exclusion list)
22:12:58.64 +38:26:20.3 -- not an asteroid (will add it to exclusion list)
21:18:40.03 +39:14:36.1 -- not an asteroid (will add it to exclusion list)
21:41:29.15 +37:46:45.6 -- not an asteroid (will add it to exclusion list)
21:32:54.35 +35:30:10.4 -- not an asteroid (will add it to exclusion list)
21:20:46.72 +33:50:41.5 -- not an asteroid (will add it to exclusion list)
21:39:07.89 +36:52:27.7 -- not an asteroid (will add it to exclusion list)
22:07:50.36 +40:07:28.2 -- not an asteroid (will add it to exclusion list)
21:48:53.62 +40:38:12.4 -- not an asteroid (will add it to exclusion list)
21:19:36.10 +38:11:41.1 -- not an asteroid (will add it to exclusion list)
21:35:30.51 +34:46:53.2 -- not an asteroid (will add it to exclusion list)
21:22:57.16 +34:21:06.6 -- not an asteroid (will add it to exclusion list)
21:55:05.31 +34:46:30.7 -- not an asteroid (will add it to exclusion list)
21:58:07.76 +38:56:42.0 -- not an asteroid (will add it to exclusion list)
22:01:49.89 +36:55:26.7 -- not an asteroid (will add it to exclusion list)
22:06:46.19 +39:39:09.6 -- not an asteroid (will add it to exclusion list)
21:42:50.12 +38:10:45.9 -- not an asteroid (will add it to exclusion list)
21:42:06.19 +36:50:53.8 -- not an asteroid (will add it to exclusion list)
22:11:23.05 +39:44:15.2 -- not an asteroid (will add it to exclusion list)
21:26:53.38 +34:58:18.2 -- not an asteroid (will add it to exclusion list)
22:13:05.31 +41:48:40.8 -- not an asteroid (will add it to exclusion list)
22:00:54.57 +41:16:15.2 -- not an asteroid (will add it to exclusion list)
21:42:21.28 +34:05:46.6 -- not an asteroid (will add it to exclusion list)
21:39:20.65 +35:38:18.7 -- not an asteroid (will add it to exclusion list)
21:44:49.77 +36:56:55.7 -- not an asteroid (will add it to exclusion list)
21:49:54.58 +34:54:44.0 -- not an asteroid (will add it to exclusion list)
21:50:52.30 +39:37:43.0 -- not an asteroid (will add it to exclusion list)
22:04:00.09 +39:46:41.1 -- not an asteroid (will add it to exclusion list)
22:21:21.26 +41:17:36.3 -- not an asteroid (will add it to exclusion list)
21:23:19.64 +35:13:30.0 -- not an asteroid (will add it to exclusion list)
22:16:38.13 +41:45:37.6 -- not an asteroid (will add it to exclusion list)
22:02:40.25 +38:06:45.2 -- not an asteroid (will add it to exclusion list)
21:59:02.61 +37:17:54.7 -- not an asteroid (will add it to exclusion list)
22:13:03.63 +38:28:17.9 -- not an asteroid (will add it to exclusion list)
21:39:39.54 +39:57:28.3 -- not an asteroid (will add it to exclusion list)
21:21:16.92 +34:59:15.3 -- not an asteroid (will add it to exclusion list)
21:57:20.62 +40:57:00.4 -- not an asteroid (will add it to exclusion list)
22:06:31.79 +34:33:33.0 -- not an asteroid (will add it to exclusion list)
21:27:05.58 +36:00:32.0 -- not an asteroid (will add it to exclusion list)
21:20:36.26 +35:29:43.0 -- not an asteroid (will add it to exclusion list)
21:36:04.29 +41:56:44.6 -- not an asteroid (will add it to exclusion list)
21:54:04.37 +37:39:41.1 -- not an asteroid (will add it to exclusion list)
21:52:31.17 +41:28:58.3 -- not an asteroid (will add it to exclusion list)
21:43:16.93 +40:27:46.9 -- not an asteroid (will add it to exclusion list)
21:35:06.90 +38:39:19.6 -- not an asteroid (will add it to exclusion list)
22:02:27.76 +42:04:01.6 -- not an asteroid (will add it to exclusion list)
21:18:30.05 +39:08:10.7 -- not an asteroid (will add it to exclusion list)
21:50:11.57 +35:33:08.5 -- not an asteroid (will add it to exclusion list)
21:38:09.28 +38:56:17.1 -- not an asteroid (will add it to exclusion list)
22:09:46.26 +41:39:58.4 -- not an asteroid (will add it to exclusion list)
21:27:48.41 +38:33:03.8 -- not an asteroid (will add it to exclusion list)
21:46:21.76 +39:50:08.5 -- not an asteroid (will add it to exclusion list)
21:49:12.20 +34:20:08.5 -- not an asteroid (will add it to exclusion list)
21:21:51.04 +37:53:26.0 -- not an asteroid (will add it to exclusion list)
21:41:09.87 +36:39:08.8 -- not an asteroid (will add it to exclusion list)
21:43:32.06 +38:44:15.1 -- not an asteroid (will add it to exclusion list)
21:43:30.47 +41:30:12.3 -- not an asteroid (will add it to exclusion list)
21:22:07.84 +36:03:45.4 -- not an asteroid (will add it to exclusion list)
21:49:54.43 +37:45:56.6 -- not an asteroid (will add it to exclusion list)
21:34:12.43 +39:03:18.4 -- not an asteroid (will add it to exclusion list)
21:57:34.03 +41:27:52.3 -- not an asteroid (will add it to exclusion list)
21:39:00.67 +38:41:34.2 -- not an asteroid (will add it to exclusion list)
21:26:29.31 +39:08:36.1 -- not an asteroid (will add it to exclusion list)
22:05:11.32 +39:28:34.7 -- not an asteroid (will add it to exclusion list)
21:58:43.28 +42:11:58.3 -- not an asteroid (will add it to exclusion list)
22:05:42.75 +35:53:01.3 -- not an asteroid (will add it to exclusion list)
21:51:54.98 +33:54:39.2 -- not an asteroid (will add it to exclusion list)
21:56:45.17 +36:22:45.2 -- not an asteroid (will add it to exclusion list)
21:32:57.30 +38:12:17.6 -- not an asteroid (will add it to exclusion list)
21:36:34.05 +37:11:49.1 -- not an asteroid (will add it to exclusion list)
22:13:03.64 +38:27:56.2 -- not an asteroid (will add it to exclusion list)
21:40:39.17 +41:35:37.9 -- not an asteroid (will add it to exclusion list)
21:29:19.08 +40:28:36.3 -- not an asteroid (will add it to exclusion list)
22:10:19.95 +38:44:17.5 -- not an asteroid (will add it to exclusion list)
21:31:28.76 +34:33:30.8 -- not an asteroid (will add it to exclusion list)
22:15:17.59 +39:47:56.7 -- not an asteroid (will add it to exclusion list)
21:23:16.30 +35:12:48.0 -- not an asteroid (will add it to exclusion list)
21:30:29.32 +34:39:52.2 -- not an asteroid (will add it to exclusion list)
21:58:13.58 +38:26:16.0 -- not an asteroid (will add it to exclusion list)
21:36:06.03 +34:59:43.1 -- not an asteroid (will add it to exclusion list)
22:00:00.17 +38:42:22.9 -- not an asteroid (will add it to exclusion list)
21:46:36.46 +37:39:35.6 -- not an asteroid (will add it to exclusion list)
21:36:02.24 +39:50:06.7 -- not an asteroid (will add it to exclusion list)
21:25:10.35 +36:09:27.9 -- not an asteroid (will add it to exclusion list)
22:18:15.73 +40:51:52.2 -- not an asteroid (will add it to exclusion list)
21:38:38.15 +33:58:30.9 -- not an asteroid (will add it to exclusion list)
21:57:15.92 +39:56:53.4 -- not an asteroid (will add it to exclusion list)
21:58:15.48 +41:40:34.6 -- not an asteroid (will add it to exclusion list)
21:40:29.72 +38:25:54.2 -- not an asteroid (will add it to exclusion list)
22:06:29.39 +39:42:25.0 -- not an asteroid (will add it to exclusion list)
21:40:27.72 +38:25:55.7 -- not an asteroid (will add it to exclusion list)
21:59:28.75 +37:59:45.7 -- not an asteroid (will add it to exclusion list)
21:49:18.24 +39:21:11.7 -- not an asteroid (will add it to exclusion list)
21:41:04.40 +37:19:14.5 -- not an asteroid (will add it to exclusion list)
22:06:04.07 +39:59:11.7 -- not an asteroid (will add it to exclusion list)
21:50:28.68 +37:17:46.6 -- not an asteroid (will add it to exclusion list)
21:30:51.99 +34:46:06.8 -- not an asteroid (will add it to exclusion list)
22:09:33.53 +41:54:58.7 -- not an asteroid (will add it to exclusion list)
22:02:05.77 +41:42:42.2 -- not an asteroid (will add it to exclusion list)
21:59:01.70 +36:26:59.5 -- not an asteroid (will add it to exclusion list)
21:25:29.43 +34:45:43.1 -- not an asteroid (will add it to exclusion list)
22:01:20.22 +41:45:33.5 -- not an asteroid (will add it to exclusion list)
21:34:26.09 +38:30:21.9 -- not an asteroid (will add it to exclusion list)
21:28:25.42 +36:06:47.3 -- not an asteroid (will add it to exclusion list)
21:48:08.06 +39:26:19.1 -- not an asteroid (will add it to exclusion list)
21:42:24.50 +38:38:04.2 -- not an asteroid (will add it to exclusion list)
21:43:03.31 +37:32:30.8 -- not an asteroid (will add it to exclusion list)
22:09:11.53 +36:46:06.5 -- not an asteroid (will add it to exclusion list)
21:37:55.53 +36:14:19.2 -- not an asteroid (will add it to exclusion list)
21:38:09.00 +35:14:31.3 -- not an asteroid (will add it to exclusion list)
21:21:10.26 +36:46:15.2 -- not an asteroid (will add it to exclusion list)
22:14:42.67 +40:16:53.2 -- not an asteroid (will add it to exclusion list)
21:19:39.27 +36:58:21.7 -- not an asteroid (will add it to exclusion list)
21:57:59.38 +41:37:14.4 -- not an asteroid (will add it to exclusion list)
21:38:09.35 +36:54:29.2 -- not an asteroid (will add it to exclusion list)
22:04:36.75 +38:54:16.0 -- not an asteroid (will add it to exclusion list)
21:41:14.37 +36:39:28.2 -- not an asteroid (will add it to exclusion list)
21:42:34.24 +37:51:57.3 -- not an asteroid (will add it to exclusion list)
21:21:48.92 +38:58:05.6 -- not an asteroid (will add it to exclusion list)
21:46:54.04 +39:15:20.6 -- not an asteroid (will add it to exclusion list)
21:56:00.61 +37:10:56.4 -- not an asteroid (will add it to exclusion list)
21:20:39.42 +35:23:14.4 -- not an asteroid (will add it to exclusion list)
21:36:33.98 +38:12:28.3 -- not an asteroid (will add it to exclusion list)
21:36:24.13 +40:56:09.6 -- not an asteroid (will add it to exclusion list)
21:46:38.60 +37:23:34.7 -- not an asteroid (will add it to exclusion list)
21:50:17.52 +42:04:58.0 -- not an asteroid (will add it to exclusion list)
21:47:31.21 +37:36:06.6 -- not an asteroid (will add it to exclusion list)
21:24:44.54 +39:07:52.7 -- not an asteroid (will add it to exclusion list)
21:23:35.30 +37:36:36.8 -- not an asteroid (will add it to exclusion list)
21:51:39.58 +42:01:59.2 -- not an asteroid (will add it to exclusion list)
21:54:53.03 +41:29:33.8 -- not an asteroid (will add it to exclusion list)
21:35:29.49 +39:47:59.8 -- not an asteroid (will add it to exclusion list)
21:23:17.77 +34:21:30.8 -- not an asteroid (will add it to exclusion list)
21:56:43.39 +41:51:09.4 -- not an asteroid (will add it to exclusion list)
21:23:15.04 +39:36:00.3 -- not an asteroid (will add it to exclusion list)
21:52:16.24 +41:27:10.3 -- not an asteroid (will add it to exclusion list)
21:49:05.08 +37:22:34.2 -- not an asteroid (will add it to exclusion list)
21:42:54.70 +40:43:52.5 -- not an asteroid (will add it to exclusion list)
21:36:32.75 +39:08:53.3 -- not an asteroid (will add it to exclusion list)
21:45:18.26 +37:39:35.7 -- not an asteroid (will add it to exclusion list)
21:50:24.88 +41:23:23.5 -- not an asteroid (will add it to exclusion list)
21:35:34.25 +34:35:51.5 -- not an asteroid (will add it to exclusion list)
22:03:42.56 +35:43:46.5 -- not an asteroid (will add it to exclusion list)
21:56:38.07 +36:20:34.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:18:16.76 +37:55:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:26.49 +38:35:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:30.05 +39:08:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:40.03 +39:14:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:47.35 +38:10:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:17.68 +37:56:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:18.67 +37:19:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:36.10 +38:11:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:39.27 +36:58:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:57.19 +39:52:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:00.19 +38:24:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:08.98 +38:06:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:26.99 +35:31:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:31.14 +38:20:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:36.26 +35:29:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:39.42 +35:23:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:46.72 +33:50:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:10.26 +36:46:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:16.92 +34:59:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:46.40 +35:01:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:48.92 +38:58:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:51.04 +37:53:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:07.84 +36:03:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:16.36 +36:13:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:26.13 +37:11:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:31.09 +37:35:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:46.56 +34:59:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:57.16 +34:21:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:57.47 +38:21:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:15.04 +39:36:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:16.30 +35:12:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:17.77 +34:21:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:19.64 +35:13:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:31.33 +39:22:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:35.30 +37:36:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:53.58 +35:33:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:57.85 +34:02:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:39.85 +33:48:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:44.54 +39:07:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:50.19 +39:27:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:10.35 +36:09:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:29.43 +34:45:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:35.29 +34:11:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:04.93 +37:38:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:29.31 +39:08:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:53.38 +34:58:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:05.58 +36:00:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:24.07 +36:58:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:41.77 +38:45:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:46.08 +35:33:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:48.41 +38:33:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:02.73 +38:25:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:09.28 +41:14:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:25.42 +36:06:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:47.08 +42:05:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:19.08 +40:28:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:29.32 +34:39:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:47.82 +38:57:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:51.99 +34:46:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.81 +39:26:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.96 +36:19:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.76 +34:33:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:29.29 +40:58:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:35.18 +38:09:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:37.92 +34:11:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:46.01 +37:06:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:48.46 +39:29:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:54.35 +35:30:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:57.30 +38:12:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:36.34 +38:32:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:12.43 +39:03:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:15.55 +38:14:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:26.09 +38:30:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:26.75 +41:42:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:04.78 +40:51:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:06.90 +38:39:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:29.49 +39:47:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:30.51 +34:46:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:34.25 +34:35:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:02.24 +39:50:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:04.29 +41:56:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:06.03 +34:59:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:24.13 +40:56:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:32.75 +39:08:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:33.98 +38:12:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:34.05 +37:11:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:55.53 +36:14:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:09.00 +35:14:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:09.28 +38:56:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:09.35 +36:54:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:38.15 +33:58:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:44.95 +35:57:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:00.67 +38:41:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:05.39 +36:51:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:07.89 +36:52:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:13.08 +42:06:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:20.65 +35:38:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:25.90 +41:43:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:39.54 +39:57:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:12.85 +36:18:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:27.72 +38:25:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:29.72 +38:25:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:39.17 +41:35:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:04.40 +37:19:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:09.87 +36:39:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:14.37 +36:39:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:28.51 +41:30:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:29.15 +37:46:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:45.14 +37:40:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:06.19 +36:50:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:21.28 +34:05:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:24.50 +38:38:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:34.24 +37:51:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:50.12 +38:10:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:50.27 +37:29:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:54.70 +40:43:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:55.14 +41:10:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:03.31 +37:32:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:05.23 +41:29:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:16.93 +40:27:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:30.47 +41:30:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:32.06 +38:44:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.38 +38:02:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:39.07 +41:53:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:49.77 +36:56:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:52.81 +37:32:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:18.26 +37:39:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:28.84 +42:12:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:43.36 +41:42:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:53.74 +35:13:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:21.76 +39:50:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:27.10 +42:00:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:36.46 +37:39:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:38.60 +37:23:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:54.04 +39:15:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:31.21 +37:36:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:50.79 +40:31:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:52.58 +34:30:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:57.33 +36:35:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:08.06 +39:26:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:18.10 +41:54:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:53.62 +40:38:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:05.08 +37:22:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:12.20 +34:20:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:18.24 +39:21:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:38.29 +41:30:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:54.43 +37:45:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:54.58 +34:54:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:11.57 +35:33:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:17.52 +42:04:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:24.88 +41:23:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:28.68 +37:17:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:52.30 +39:37:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:55.94 +34:03:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.58 +42:01:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:52.25 +41:19:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:54.98 +33:54:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:09.56 +38:58:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:16.24 +41:27:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:31.17 +41:28:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:53.73 +41:17:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:04.37 +37:39:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:25.00 +39:39:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:53.03 +41:29:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:05.31 +34:46:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:20.92 +40:52:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.61 +37:10:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:37.89 +37:20:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:38.07 +36:20:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:43.39 +41:51:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:45.17 +36:22:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:58.95 +36:20:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:15.92 +39:56:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:20.62 +40:57:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:22.83 +40:56:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:34.03 +41:27:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:59.38 +41:37:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:07.76 +38:56:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:13.58 +38:26:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:15.48 +41:40:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:37.13 +33:56:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:43.28 +42:11:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:48.44 +41:41:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:01.70 +36:26:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:02.61 +37:17:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:28.75 +37:59:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:00.17 +38:42:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:14.39 +41:40:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:54.57 +41:16:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:20.22 +41:45:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:49.89 +36:55:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:05.77 +41:42:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:27.76 +42:04:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:40.25 +38:06:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:54.19 +40:52:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:42.56 +35:43:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:59.00 +40:08:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:00.09 +39:46:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:36.75 +38:54:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:11.32 +39:28:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:42.75 +35:53:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:04.07 +39:59:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:29.39 +39:42:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:31.79 +34:33:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:46.19 +39:39:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:50.36 +40:07:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:33.83 +41:26:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:11.53 +36:46:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:33.53 +41:54:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:46.26 +41:39:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:19.95 +38:44:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:23.05 +39:44:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:51.18 +39:09:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:58.64 +38:26:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:03.63 +38:28:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:03.64 +38:27:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:05.31 +41:48:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:14.65 +41:47:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:41.76 +40:56:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:42.67 +40:16:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:11.65 +39:02:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:17.59 +39:47:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:38.13 +41:45:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:15.73 +40:51:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:21.26 +41:17:36.3 -- 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)
21:18:16.76 +37:55:32.6 -- a known variable star
21:18:26.49 +38:35:23.1 -- not a known variable star
21:18:30.05 +39:08:10.7 -- not a known variable star
21:18:40.03 +39:14:36.1 -- not a known variable star
21:18:47.35 +38:10:22.2 -- a known variable star
21:19:17.68 +37:56:05.4 -- not a known variable star
21:19:18.67 +37:19:00.9 -- not a known variable star
21:19:36.10 +38:11:41.1 -- a known variable star
21:19:39.27 +36:58:21.7 -- a known variable star
21:19:57.19 +39:52:25.7 -- not a known variable star
21:20:00.19 +38:24:37.2 -- a known variable star
21:20:08.98 +38:06:51.3 -- not a known variable star
21:20:26.99 +35:31:37.1 -- not a known variable star
21:20:31.14 +38:20:14.1 -- not a known variable star
21:20:36.26 +35:29:43.0 -- not a known variable star
21:20:39.42 +35:23:14.4 -- not a known variable star
21:20:46.72 +33:50:41.5 -- not a known variable star
21:21:10.26 +36:46:15.2 -- not a known variable star
21:21:16.92 +34:59:15.3 -- not a known variable star
21:21:46.40 +35:01:45.8 -- a known variable star
21:21:48.92 +38:58:05.6 -- not a known variable star
21:21:51.04 +37:53:26.0 -- not a known variable star
21:22:07.84 +36:03:45.4 -- a known variable star
21:22:16.36 +36:13:44.9 -- not a known variable star
21:22:26.13 +37:11:04.3 -- not a known variable star
21:22:31.09 +37:35:51.7 -- not a known variable star
21:22:46.56 +34:59:22.5 -- not a known variable star
21:22:57.16 +34:21:06.6 -- not a known variable star
21:22:57.47 +38:21:11.6 -- not a known variable star
21:23:15.04 +39:36:00.3 -- not a known variable star
21:23:16.30 +35:12:48.0 -- not a known variable star
21:23:17.77 +34:21:30.8 -- not a known variable star
21:23:19.64 +35:13:30.0 -- not a known variable star
21:23:31.33 +39:22:16.0 -- not a known variable star
21:23:35.30 +37:36:36.8 -- not a known variable star
21:23:53.58 +35:33:45.7 -- not a known variable star
21:23:57.85 +34:02:50.2 -- not a known variable star
21:24:39.85 +33:48:21.5 -- not a known variable star
21:24:44.54 +39:07:52.7 -- not a known variable star
21:24:50.19 +39:27:06.1 -- not a known variable star
21:25:10.35 +36:09:27.9 -- not a known variable star
21:25:29.43 +34:45:43.1 -- a known variable star
21:25:35.29 +34:11:53.2 -- a known variable star
21:26:04.93 +37:38:02.0 -- not a known variable star
21:26:29.31 +39:08:36.1 -- a known variable star
21:26:53.38 +34:58:18.2 -- not a known variable star
21:27:05.58 +36:00:32.0 -- not a known variable star
21:27:24.07 +36:58:25.0 -- not a known variable star
21:27:41.77 +38:45:45.4 -- not a known variable star
21:27:46.08 +35:33:54.1 -- not a known variable star
21:27:48.41 +38:33:03.8 -- not a known variable star
21:28:02.73 +38:25:44.9 -- not a known variable star
21:28:09.28 +41:14:36.0 -- not a known variable star
21:28:25.42 +36:06:47.3 -- not a known variable star
21:28:47.08 +42:05:19.1 -- not a known variable star
21:29:19.08 +40:28:36.3 -- not a known variable star
21:30:29.32 +34:39:52.2 -- not a known variable star
21:30:47.82 +38:57:32.5 -- not a known variable star
21:30:51.99 +34:46:06.8 -- not a known variable star
21:31:14.81 +39:26:58.6 -- a known variable star
21:31:14.96 +36:19:50.3 -- not a known variable star
21:31:28.76 +34:33:30.8 -- not a known variable star
21:31:29.29 +40:58:23.7 -- a known variable star
21:31:35.18 +38:09:23.1 -- not a known variable star
21:31:37.92 +34:11:28.6 -- not a known variable star
21:32:46.01 +37:06:20.5 -- not a known variable star
21:32:48.46 +39:29:41.6 -- not a known variable star
21:32:54.35 +35:30:10.4 -- not a known variable star
21:32:57.30 +38:12:17.6 -- not a known variable star
21:33:36.34 +38:32:50.2 -- not a known variable star
21:34:12.43 +39:03:18.4 -- not a known variable star
21:34:15.55 +38:14:21.3 -- not a known variable star
21:34:26.09 +38:30:21.9 -- a known variable star
21:34:26.75 +41:42:34.0 -- not a known variable star
21:35:04.78 +40:51:23.3 -- a known variable star
21:35:06.90 +38:39:19.6 -- a known variable star
21:35:29.49 +39:47:59.8 -- not a known variable star
21:35:30.51 +34:46:53.2 -- not a known variable star
21:35:34.25 +34:35:51.5 -- not a known variable star
21:36:02.24 +39:50:06.7 -- not a known variable star
21:36:04.29 +41:56:44.6 -- not a known variable star
21:36:06.03 +34:59:43.1 -- not a known variable star
21:36:24.13 +40:56:09.6 -- not a known variable star
21:36:32.75 +39:08:53.3 -- not a known variable star
21:36:33.98 +38:12:28.3 -- not a known variable star
21:36:34.05 +37:11:49.1 -- a known variable star
21:37:55.53 +36:14:19.2 -- not a known variable star
21:38:09.00 +35:14:31.3 -- not a known variable star
21:38:09.28 +38:56:17.1 -- not a known variable star
21:38:09.35 +36:54:29.2 -- not a known variable star
21:38:38.15 +33:58:30.9 -- not a known variable star
21:38:44.95 +35:57:35.2 -- a known variable star
21:39:00.67 +38:41:34.2 -- not a known variable star
21:39:05.39 +36:51:24.2 -- not a known variable star
21:39:07.89 +36:52:27.7 -- not a known variable star
21:39:13.08 +42:06:32.0 -- a known variable star
21:39:20.65 +35:38:18.7 -- not a known variable star
21:39:25.90 +41:43:13.8 -- not a known variable star
21:39:39.54 +39:57:28.3 -- not a known variable star
21:40:12.85 +36:18:00.6 -- not a known variable star
21:40:27.72 +38:25:55.7 -- a known variable star
21:40:29.72 +38:25:54.2 -- a known variable star
21:40:39.17 +41:35:37.9 -- not a known variable star
21:41:04.40 +37:19:14.5 -- not a known variable star
21:41:09.87 +36:39:08.8 -- a known variable star
21:41:14.37 +36:39:28.2 -- not a known variable star
21:41:28.51 +41:30:43.6 -- not a known variable star
21:41:29.15 +37:46:45.6 -- not a known variable star
21:41:45.14 +37:40:54.2 -- not a known variable star
21:42:06.19 +36:50:53.8 -- not a known variable star
21:42:21.28 +34:05:46.6 -- not a known variable star
21:42:24.50 +38:38:04.2 -- not a known variable star
21:42:34.24 +37:51:57.3 -- not a known variable star
21:42:50.12 +38:10:45.9 -- not a known variable star
21:42:50.27 +37:29:32.7 -- a known variable star
21:42:54.70 +40:43:52.5 -- not a known variable star
21:42:55.14 +41:10:20.0 -- not a known variable star
21:43:03.31 +37:32:30.8 -- not a known variable star
21:43:05.23 +41:29:28.1 -- not a known variable star
21:43:16.93 +40:27:46.9 -- not a known variable star
21:43:30.47 +41:30:12.3 -- not a known variable star
21:43:32.06 +38:44:15.1 -- not a known variable star
21:44:37.38 +38:02:19.2 -- not a known variable star
21:44:39.07 +41:53:49.7 -- not a known variable star
21:44:49.77 +36:56:55.7 -- not a known variable star
21:44:52.81 +37:32:27.1 -- not a known variable star
21:45:18.26 +37:39:35.7 -- not a known variable star
21:45:28.84 +42:12:24.4 -- not a known variable star
21:45:43.36 +41:42:23.0 -- not a known variable star
21:45:53.74 +35:13:19.2 -- not a known variable star
21:46:21.76 +39:50:08.5 -- not a known variable star
21:46:27.10 +42:00:03.0 -- not a known variable star
21:46:36.46 +37:39:35.6 -- not a known variable star
21:46:38.60 +37:23:34.7 -- not a known variable star
21:46:54.04 +39:15:20.6 -- not a known variable star
21:47:31.21 +37:36:06.6 -- not a known variable star
21:47:50.79 +40:31:46.2 -- not a known variable star
21:47:52.58 +34:30:12.8 -- not a known variable star
21:47:57.33 +36:35:33.9 -- not a known variable star
21:48:08.06 +39:26:19.1 -- not a known variable star
21:48:18.10 +41:54:23.7 -- not a known variable star
21:48:53.62 +40:38:12.4 -- not a known variable star
21:49:05.08 +37:22:34.2 -- not a known variable star
21:49:12.20 +34:20:08.5 -- not a known variable star
21:49:18.24 +39:21:11.7 -- not a known variable star
21:49:38.29 +41:30:55.0 -- a known variable star
21:49:54.43 +37:45:56.6 -- not a known variable star
21:49:54.58 +34:54:44.0 -- not a known variable star
21:50:11.57 +35:33:08.5 -- a known variable star
21:50:17.52 +42:04:58.0 -- a known variable star
21:50:24.88 +41:23:23.5 -- not a known variable star
21:50:28.68 +37:17:46.6 -- not a known variable star
21:50:52.30 +39:37:43.0 -- not a known variable star
21:50:55.94 +34:03:39.1 -- not a known variable star
21:51:39.58 +42:01:59.2 -- not a known variable star
21:51:52.25 +41:19:33.8 -- not a known variable star
21:51:54.98 +33:54:39.2 -- not a known variable star
21:52:09.56 +38:58:10.1 -- not a known variable star
21:52:16.24 +41:27:10.3 -- not a known variable star
21:52:31.17 +41:28:58.3 -- not a known variable star
21:53:53.73 +41:17:51.7 -- not a known variable star
21:54:04.37 +37:39:41.1 -- not a known variable star
21:54:25.00 +39:39:27.7 -- not a known variable star
21:54:53.03 +41:29:33.8 -- a known variable star
21:55:05.31 +34:46:30.7 -- not a known variable star
21:55:20.92 +40:52:13.1 -- not a known variable star
21:56:00.61 +37:10:56.4 -- not a known variable star
21:56:37.89 +37:20:32.3 -- not a known variable star
21:56:38.07 +36:20:34.7 -- a known variable star
21:56:43.39 +41:51:09.4 -- not a known variable star
21:56:45.17 +36:22:45.2 -- not a known variable star
21:56:58.95 +36:20:20.9 -- a known variable star
21:57:15.92 +39:56:53.4 -- not a known variable star
21:57:20.62 +40:57:00.4 -- not a known variable star
21:57:22.83 +40:56:51.4 -- not a known variable star
21:57:34.03 +41:27:52.3 -- not a known variable star
21:57:59.38 +41:37:14.4 -- not a known variable star
21:58:07.76 +38:56:42.0 -- not a known variable star
21:58:13.58 +38:26:16.0 -- not a known variable star
21:58:15.48 +41:40:34.6 -- not a known variable star
21:58:37.13 +33:56:11.7 -- a known variable star
21:58:43.28 +42:11:58.3 -- not a known variable star
21:58:48.44 +41:41:43.3 -- not a known variable star
21:59:01.70 +36:26:59.5 -- not a known variable star
21:59:02.61 +37:17:54.7 -- not a known variable star
21:59:28.75 +37:59:45.7 -- not a known variable star
22:00:00.17 +38:42:22.9 -- a known variable star
22:00:14.39 +41:40:34.0 -- not a known variable star
22:00:54.57 +41:16:15.2 -- not a known variable star
22:01:20.22 +41:45:33.5 -- a known variable star
22:01:49.89 +36:55:26.7 -- not a known variable star
22:02:05.77 +41:42:42.2 -- not a known variable star
22:02:27.76 +42:04:01.6 -- not a known variable star
22:02:40.25 +38:06:45.2 -- not a known variable star
22:02:54.19 +40:52:41.4 -- not a known variable star
22:03:42.56 +35:43:46.5 -- a known variable star
22:03:59.00 +40:08:16.2 -- a known variable star
22:04:00.09 +39:46:41.1 -- not a known variable star
22:04:36.75 +38:54:16.0 -- not a known variable star
22:05:11.32 +39:28:34.7 -- not a known variable star
22:05:42.75 +35:53:01.3 -- not a known variable star
22:06:04.07 +39:59:11.7 -- not a known variable star
22:06:29.39 +39:42:25.0 -- not a known variable star
22:06:31.79 +34:33:33.0 -- not a known variable star
22:06:46.19 +39:39:09.6 -- not a known variable star
22:07:50.36 +40:07:28.2 -- not a known variable star
22:08:33.83 +41:26:35.6 -- not a known variable star
22:09:11.53 +36:46:06.5 -- not a known variable star
22:09:33.53 +41:54:58.7 -- not a known variable star
22:09:46.26 +41:39:58.4 -- not a known variable star
22:10:19.95 +38:44:17.5 -- a known variable star
22:11:23.05 +39:44:15.2 -- not a known variable star
22:12:51.18 +39:09:59.3 -- a known variable star
22:12:58.64 +38:26:20.3 -- a known variable star
22:13:03.63 +38:28:17.9 -- not a known variable star
22:13:03.64 +38:27:56.2 -- not a known variable star
22:13:05.31 +41:48:40.8 -- not a known variable star
22:13:14.65 +41:47:42.9 -- not a known variable star
22:13:41.76 +40:56:39.1 -- not a known variable star
22:14:42.67 +40:16:53.2 -- not a known variable star
22:15:11.65 +39:02:25.1 -- not a known variable star
22:15:17.59 +39:47:56.7 -- not a known variable star
22:16:38.13 +41:45:37.6 -- not a known variable star
22:18:15.73 +40:51:52.2 -- not a known variable star
22:21:21.26 +41:17:36.3 -- not a known variable star
Found 189 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
225 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 225 (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)2461120.94916341 -observatory 500
22:37:55.41 -07:44:36.1 Mercury (1.0mag)
01:08:37.22 +06:22:29.2 Venus (-3.9mag)
23:04:28.73 -07:06:05.7 Mars (1.2mag)
07:04:49.56 +22:57:56.2 Jupiter (-2.3mag)
00:17:33.27 -00:24:50.8 Saturn (0.9mag)
03:43:00.22 +19:32:06.2 Uranus (5.8mag)
00:07:21.15 -00:37:38.0 Neptune (7.8mag)
20:32:02.73 -22:53:44.1 Pluto (14.5mag)
01:53:51.36 +16:10:40.8 Moon (-8.9mag)
-rw-r--r-- 1 apache apache 361 Mar 21 05:50 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461120.94916341:
07:04:47.95 +22:57:56.0 Io (5.6mag)
07:04:38.18 +22:58:19.9 Europa (5.7mag)
07:04:27.62 +22:58:37.4 Ganymede (5.2mag)
07:04:12.34 +22:59:01.7 Callisto (6.4mag)
07:08:50.78 +22:59:17.3 Himalia (15.2mag)
07:04:48.15 +22:57:55.9 Thebe (16.0mag)
07:08:26.18 +23:22:46.1 Elara (17.2mag)
07:01:59.31 +23:51:22.9 Pasiphae (17.2mag)
07:13:36.63 +22:52:28.5 Carme (18.3mag)
00:17:28.90 -00:24:48.9 Titan (8.8mag)
00:17:39.07 -00:24:48.3 Rhea (10.1mag)
00:18:02.61 -00:22:47.2 Iapetus (11.5mag)
00:17:48.53 -00:24:54.8 Hyperion (14.8mag)
00:19:27.17 -00:13:36.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 21 05:50 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461120.94916341:
12:53:38.01 +08:22:39.1 JWST
17:03:57.20 +43:58:01.7 Chandra
09:05:01.52 -48:35:07.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 21 05:50 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461120.94916341 -observatory 500
18:35:47.38 -27:28:53.7 14.0mag P/2010 H2 (Vales)
04:51:22.35 -71:00:28.2 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:45.68 +31:18:00.2 17.0mag C/2017 K2 (PANSTARRS)
17:29:42.38 +07:27:32.3 17.6mag C/2021 G2 (ATLAS)
23:01:43.99 +28:26:41.2 16.9mag C/2022 E2 (ATLAS)
04:00:57.59 +25:18:26.5 15.7mag C/2022 N2 (PANSTARRS)
09:01:50.72 +31:27:59.9 16.0mag C/2022 QE78 (ATLAS)
08:30:09.26 -03:07:15.8 17.2mag C/2022 R6 (PANSTARRS)
18:56:30.28 +16:19:48.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:18.74 -11:50:29.5 17.6mag P/2023 B1 (PANSTARRS)
09:24:09.32 -16:14:55.0 17.4mag C/2023 F3 (ATLAS)
21:22:21.95 +61:42:42.6 17.4mag C/2023 H5 (Lemmon)
19:33:05.03 -03:31:18.7 14.5mag C/2023 R1 (PANSTARRS)
21:36:44.02 +82:53:46.8 17.7mag C/2023 X2 (Lemmon)
06:15:15.28 +63:46:48.7 16.8mag C/2024 A1 (ATLAS)
04:07:51.01 +05:32:10.4 9.1mag C/2024 E1 (Wierzchos)
11:22:16.06 +02:49:10.5 18.0mag C/2024 G2 (ATLAS)
16:32:07.17 +02:14:06.7 17.5mag C/2024 G6 (ATLAS)
20:10:17.64 +08:52:00.9 14.9mag C/2024 J3 (ATLAS)
03:05:02.64 -26:34:30.2 16.5mag C/2024 T5 (ATLAS)
04:57:48.26 +52:27:48.0 17.6mag C/2025 J1 (Borisov)
15:12:33.75 +18:04:21.2 14.4mag C/2025 L1 (ATLAS)
02:49:05.16 -22:38:10.8 17.6mag C/2025 Q3 (ATLAS)
22:33:11.94 +19:02:46.5 12.4mag C/2025 R3 (PANSTARRS)
13:04:53.83 +01:20:30.9 17.6mag C/2025 Y1 (ATLAS)
02:08:40.57 -06:05:29.3 14.0mag C/2026 A1 (MAPS)
22:40:25.29 +31:10:44.1 13.7mag C/2026 B2 (Sun-Gao)
17:52:56.72 -10:49:42.0 13.3mag 10P/Tempel
15:26:33.97 +05:06:49.8 11.8mag 24P/Schaumasse
11:11:48.57 -02:27:49.5 15.6mag 29P/Schwassmann-Wachmann
17:44:07.31 -10:37:42.5 17.3mag 40P/Vaisala
10:44:55.09 -06:31:12.9 16.4mag 43P/Wolf-Harrington
01:09:38.01 +13:00:14.6 17.0mag 47P/Ashbrook-Jackson
06:29:11.70 +42:15:37.3 17.1mag 63P/Wild
22:54:49.63 -14:41:00.2 15.7mag 65P/Gunn
02:59:30.15 +11:30:33.4 15.9mag 76P/West-Kohoutek-Ikemura
00:10:27.42 +03:08:17.1 14.6mag 78P/Gehrels
21:40:17.44 -16:37:40.2 14.5mag 88P/Howell
01:01:53.69 +13:21:37.8 15.2mag 93P/Lovas
04:11:16.44 +30:42:55.5 16.5mag 123P/West-Hartley
08:07:55.28 +50:03:56.8 16.2mag 124P/Mrkos
01:54:59.02 +11:24:27.8 16.4mag 128P/Shoemaker-Holt
01:58:14.93 +11:05:49.6 17.4mag 131P/Mueller
23:22:03.73 +03:16:41.0 12.9mag 141P/Machholz
23:32:11.35 -04:17:19.4 13.0mag 141P-A/Machholz
22:32:39.21 -06:51:51.4 16.0mag 141P-D/Machholz
23:51:38.68 -13:56:31.7 15.5mag 162P/SidingSpring
10:39:02.61 +32:01:58.6 17.5mag 164P/Christensen
05:50:30.03 +24:44:09.3 17.5mag 198P/ODAS
15:32:46.44 -03:18:44.2 16.9mag 210P/Christensen
20:13:32.19 -17:27:07.5 17.2mag 218P/LINEAR
16:59:44.70 -16:38:15.1 16.3mag 235P/LINEAR
04:42:17.72 +32:03:32.4 16.3mag 240P/NEAT
07:29:57.16 -08:18:45.2 17.5mag 242P/Spahr
15:48:33.13 +05:08:14.8 17.7mag 391P/Kowalski
07:28:01.91 +21:06:53.9 17.5mag 450P/LONEOS
05:01:29.99 +46:35:17.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 21 05:50 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
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
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
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
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
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
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
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
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
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
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
-rw-r--r-- 1 apache apache 5.7K Mar 21 05:50 asassn_transients_list.txt
############################################################
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 21 05:50 tocp_transients_list.txt