This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP
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+391002,2461119.9486,10.71,0.05,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
NSVS J2212515+391002 20260320.4486 10.71CV 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/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:51.16 +39:09:59.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.44 21:36:51.86 +34:54:48.4
83.79654 -12.78173 galactic Cyg Second-epoch detections are separated by 2.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:51.86 +34:54:48.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.640+/-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
target,2461119.9486,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:51.86 +34:54:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.39 21:31:59.67 +39:17:14.9
86.13641 -8.93527 galactic Cyg Second-epoch detections are separated by 3.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:59.67 +39:17:14.9 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.9486,12.39,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:59.67 +39:17:14.9 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.25 21:27:27.09 +41:06:11.3
86.77478 -7.02492 galactic Cyg Second-epoch detections are separated by 0.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:27.09 +41:06:11.3 (user input) | T | P | (position from user input) J-Ks=0.459+/-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,2461119.9486,12.25,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:27.09 +41:06:11.3 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,12.06,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:40.47 +37:26:57.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.97,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:49.98 +35:00:32.1 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.01 21:32:27.33 +38:28:56.2
85.64038 -9.58080 galactic Cyg Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1964311887063133440 | 21:32:26.35 +38:28:21.4 (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 1964311887063133440,2461119.9486,12.01,0.05,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 1964311887063133440 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:27.33 +38:28:56.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.87,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:57.05 +36:16:51.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1964864735256226432,2461119.9486,11.94,0.05,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 1964864735256226432 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:00.07 +38:24:37.6 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.01 21:48:12.40 +41:41:12.8
90.08171 -9.20914 galactic Cyg Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1960503900338500992 | 21:48:14.24 +41:40:60.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.489+/-0.045 (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 1960503900338500992,2461119.9486,12.01,0.05,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 1960503900338500992 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:12.40 +41:41:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1972591037821053952,2461119.9486,11.89,0.05,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
Gaia DR3 1972591037821053952 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:29.64 +42:12:24.5 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.92,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:53.92 +40:49:54.0 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.76 21:20:51.21 +38:55:12.7
84.31934 -7.68094 galactic Cyg Second-epoch detections are separated by 7.4" and 4.3 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 | 21:20:51.21 +38:55:12.7 (user input) | T | P | (position from user input) J-Ks=1.496+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.9486,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260320.4486 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:51.21 +38:55:12.7 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.82 21:34:11.06 +35:48:32.9
84.02017 -11.75555 galactic Cyg Second-epoch detections are separated by 2.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950999202129732224 | 21:34:12.07 +35:47:54.8 (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 1950999202129732224,2461119.9486,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950999202129732224 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:11.06 +35:48:32.9 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:48.75 +35:04:55.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.72 21:20:26.95 +35:31:38.5
81.80221 -9.99011 galactic Cyg Second-epoch detections are separated by 1.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:20:26.95 +35:31:38.5 (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,2461119.9486,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:26.95 +35:31:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.55 21:19:57.28 +39:52:27.1
84.88380 -6.88924 galactic Cyg Second-epoch detections are separated by 2.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.9852+39.8763 | 21:19:57.28 +39:52:27.1 (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 J319.9852+39.8763,2461119.9486,11.55,0.05,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 J319.9852+39.8763 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:57.28 +39:52:27.1 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.53 21:41:19.36 +37:02:33.7
85.95252 -11.82780 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:19.36 +37:02:33.7 (user input) | T | P | (position from user input) J-Ks=0.669+/-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,2461119.9486,11.53,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:19.36 +37:02:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.51 21:22:26.02 +37:11:04.3
83.28831 -9.11934 galactic Cyg Second-epoch detections are separated by 3.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.6100+37.1872 | 21:22:26.02 +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+37.1872,2461119.9486,11.51,0.05,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 J320.6100+37.1872 20260320.4486 11.51CV 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:26.02 +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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.60 21:40:56.21 +41:13:23.5
88.73297 -8.66583 galactic Cyg Second-epoch detections are separated by 1.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2343+41.2229 | 21:40:56.21 +41:13:23.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.331+/-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 J325.2343+41.2229,2461119.9486,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2343+41.2229 20260320.4486 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:40:56.21 +41:13:23.5 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1964745159067548800,2461119.9486,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964745159067548800 20260320.4486 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:16.70 +37:55:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.03 21:46:27.04 +42:00:02.8
90.03572 -8.75812 galactic Cyg Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:27.04 +42:00:02.8 (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,2461119.9486,11.03,0.05,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
target 20260320.4486 11.03CV 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:27.04 +42:00:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 10.48 21:47:57.29 +36:35:34.2
86.66422 -13.04481 galactic Cyg Second-epoch detections are separated by 0.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 1952454543207886464,2461119.9486,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952454543207886464 20260320.4486 10.48CV 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:57.29 +36:35:34.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,10.65,0.05,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
V1907 Cyg 20260320.4486 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_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:14.69 +39:26:58.9 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.05,0.05,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
V1338 Cyg 20260320.4486 11.05CV 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:04.81 +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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.18 21:52:09.49 +38:58:10.0
88.88928 -11.77368 galactic Cyg Second-epoch detections are separated by 0.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:09.49 +38:58:10.0 (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,2461119.9486,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:09.49 +38:58:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.20,0.05,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 20260320.4486 11.20CV 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:48.39 +41:41:43.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.26 22:13:14.50 +41:47:43.5
93.90028 -11.98877 galactic Lac Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.2961+41.7989 | 22:13:14.50 +41:47:43.5 (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+41.7989,2461119.9486,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.2961+41.7989 20260320.4486 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:14.50 +41:47:43.5 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.24 21:33:36.29 +38:32:50.2
85.85131 -9.68816 galactic Cyg Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:36.29 +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,2461119.9486,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:36.29 +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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.42 21:42:55.22 +41:08:31.8
88.96146 -8.97384 galactic Cyg Second-epoch detections are separated by 0.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:55.22 +41:08:31.8 (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,2461119.9486,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:55.22 +41:08:31.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1955258748835187456,2461119.9486,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955258748835187456 20260320.4486 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:58.61 +38:26:20.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.39 21:32:54.31 +35:30:11.4
83.61233 -11.79715 galactic Cyg Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 1951363316579121152,2461119.9486,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951363316579121152 20260320.4486 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:54.31 +35:30:11.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.42 21:38:32.00 +39:29:21.8
87.21315 -9.64786 galactic Cyg Second-epoch detections are separated by 1.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.6238+39.4812 | 21:38:32.00 +39:29:21.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.841+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.6238+39.4812,2461119.9486,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.6238+39.4812 20260320.4486 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:32.00 +39:29:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.43 21:48:53.57 +40:38:12.5
89.49319 -10.09387 galactic Cyg Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.2219+40.6351 | 21:48:53.57 +40:38:12.5 (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 J327.2219+40.6351,2461119.9486,11.43,0.05,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
ATO J327.2219+40.6351 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:53.57 +40:38:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.49 21:42:50.08 +38:10:46.2
86.95480 -11.18174 galactic Cyg Second-epoch detections are separated by 0.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6987+38.1778 | 21:42:50.08 +38:10:46.2 (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+38.1778,2461119.9486,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6987+38.1778 20260320.4486 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:50.08 +38:10:46.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.55 21:42:06.12 +36:50:54.8
85.93773 -12.07625 galactic Cyg Second-epoch detections are separated by 0.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5190+36.8572 | 21:42:06.12 +36:50:54.8 (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+36.8572,2461119.9486,11.55,0.05,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 J325.5190+36.8572 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:06.12 +36:50:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.46,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:07.66 +38:56:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.44 21:24:18.17 +34:35:15.9
81.67774 -11.21068 galactic Cyg Second-epoch detections are separated by 2.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:24:18.17 +34:35:15.9 (user input) | T | P | (position from user input) J-Ks=0.640+/-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,2461119.9486,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:18.17 +34:35:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.55 21:55:05.16 +34:46:31.1
86.58408 -15.36726 galactic Peg Second-epoch detections are separated by 1.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:05.16 +34:46:31.1 (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,2461119.9486,11.55,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:05.16 +34:46:31.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.53 22:07:50.34 +40:07:29.1
92.04965 -12.73942 galactic Lac Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9519+40.1216 | 22:07:50.34 +40:07:29.1 (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+40.1216,2461119.9486,11.53,0.05,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 J331.9519+40.1216 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:50.34 +40:07:29.1 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1966543685210790528,2461119.9486,11.61,0.05,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
Gaia DR3 1966543685210790528 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:14.62 +41:17:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.69 21:57:28.46 +41:27:31.9
91.29412 -10.48558 galactic Cyg Second-epoch detections are separated by 0.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:28.46 +41:27:31.9 (user input) | T | P | (position from user input) J-Ks=0.672+/-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,2461119.9486,11.69,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:28.46 +41:27:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.54,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:05:09.89 +37:27:59.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.70 22:11:22.94 +39:44:15.4
92.37559 -13.45391 galactic Lac Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:22.94 +39:44:15.4 (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,2461119.9486,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:22.94 +39:44:15.4 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.76 21:50:52.28 +39:37:42.5
89.12609 -11.10853 galactic Cyg Second-epoch detections are separated by 0.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.7283+39.6224 | 21:50:52.28 +39:37:42.5 (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+39.6224,2461119.9486,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260320.4486 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:52.28 +39:37:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.77 21:59:27.29 +38:47:17.4
89.89880 -12.81121 galactic Lac Second-epoch detections are separated by 4.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:27.29 +38:47:17.4 (user input) | T | P | (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
target,2461119.9486,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:27.29 +38:47:17.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.65 21:35:30.50 +34:46:53.1
83.49624 -12.68667 galactic Cyg Second-epoch detections are separated by 2.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:30.50 +34:46:53.1 (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,2461119.9486,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.65CV 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_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:30.50 +34:46:53.1 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.77 21:39:39.44 +39:57:29.0
87.69470 -9.44575 galactic Cyg Second-epoch detections are separated by 0.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.9057+39.9504 | 21:39:39.44 +39:57:29.0 (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+39.9504,2461119.9486,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.9057+39.9504 20260320.4486 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:39.44 +39:57:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.86 22:09:46.33 +41:39:57.4
93.28624 -11.71560 galactic Lac Second-epoch detections are separated by 4.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1958254196465679360 | 22:09:49.52 +41:39:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958254196465679360,2461119.9486,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958254196465679360 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:46.33 +41:39:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.81 22:00:54.51 +41:16:15.5
91.69119 -11.03176 galactic Lac Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:54.51 +41:16:15.5 (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,2461119.9486,11.81,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:54.51 +41:16:15.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.84 22:02:40.05 +38:06:48.8
89.97748 -13.73037 galactic Lac Second-epoch detections are separated by 0.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.6734+38.1123 | 22:02:40.05 +38:06:48.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (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 J330.6734+38.1123,2461119.9486,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.6734+38.1123 20260320.4486 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:40.05 +38:06:48.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.73 22:01:13.37 +38:32:59.5
90.02488 -13.21220 galactic Lac Second-epoch detections are separated by 1.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2962+38.5586 | 22:01:13.37 +38:32:59.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.341+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2962+38.5586,2461119.9486,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.2962+38.5586 20260320.4486 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:13.37 +38:32:59.5 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.78 21:46:21.84 +39:50:09.2
88.59145 -10.38875 galactic Cyg Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:21.84 +39:50:09.2 (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,2461119.9486,11.78,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:21.84 +39:50:09.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.82 21:39:20.67 +35:38:19.5
84.68291 -12.59589 galactic Cyg Second-epoch detections are separated by 0.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:20.67 +35:38:19.5 (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,2461119.9486,11.82,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:20.67 +35:38:19.5 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.85,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:59.93 +39:46:40.3 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.83 22:13:05.26 +41:48:42.1
93.88602 -11.95887 galactic Lac Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:13:05.26 +41:48:42.1 (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,2461119.9486,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:05.26 +41:48:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.85 21:31:09.91 +36:52:32.6
84.32471 -10.56477 galactic Cyg Second-epoch detections are separated by 2.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.7961+36.8669 | 21:31:09.91 +36:52:32.6 (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 J322.7961+36.8669,2461119.9486,11.85,0.05,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 J322.7961+36.8669 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:09.91 +36:52:32.6 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.88 21:41:13.46 +41:18:24.1
88.82994 -8.63936 galactic Cyg Second-epoch detections are separated by 2.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3034+41.3079 | 21:41:13.46 +41:18:24.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.689+/-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 J325.3034+41.3079,2461119.9486,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3034+41.3079 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:13.46 +41:18:24.1 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.89 21:36:04.27 +41:56:43.7
88.54029 -7.51994 galactic Cyg Second-epoch detections are separated by 4.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.0150+41.9494 | 21:36:04.27 +41:56:43.7 (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 J324.0150+41.9494,2461119.9486,11.89,0.05,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 J324.0150+41.9494 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:04.27 +41:56:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1953787774078443136,2461119.9486,11.94,0.05,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 1953787774078443136 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:02.70 +39:00:12.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.97 21:57:20.63 +40:57:00.9
90.95189 -10.86791 galactic Cyg Second-epoch detections are separated by 1.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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+40.9483,2461119.9486,11.97,0.05,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 J329.3425+40.9483 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:20.63 +40:57:00.9 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.81 21:41:14.17 +41:15:47.8
88.80245 -8.67329 galactic Cyg Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3088+41.2622 | 21:41:14.17 +41:15:47.8 (user input) | MSINE (ATLAS) | (ATLAS) | (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
ATO J325.3088+41.2622,2461119.9486,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3088+41.2622 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:14.17 +41:15:47.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.94 21:38:09.12 +38:56:14.9
86.78018 -10.00572 galactic Cyg Second-epoch detections are separated by 5.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5358+38.9323 | 21:38:09.12 +38:56:14.9 (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 J324.5358+38.9323,2461119.9486,11.94,0.05,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 J324.5358+38.9323 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:09.12 +38:56:14.9 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.89 21:44:17.21 +39:14:05.5
87.88286 -10.57888 galactic Cyg Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.0806+39.2316 | 21:44:17.21 +39:14:05.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.463+/-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 J326.0806+39.2316,2461119.9486,11.89,0.05,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 J326.0806+39.2316 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:17.21 +39:14:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.87 21:20:02.44 +34:06:12.1
80.69928 -10.91661 galactic Cyg Second-epoch detections are separated by 3.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1855232018531837184 | 21:20:05.03 +34:06:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.672+/-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
Gaia DR3 1855232018531837184,2461119.9486,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1855232018531837184 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:02.44 +34:06:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.90,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:49.63 +36:56:56.7 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.86,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:54.51 +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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.91,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:15.79 +35:12:51.0 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.96 22:02:27.65 +42:04:05.5
92.42095 -10.57815 galactic Lac Second-epoch detections are separated by 1.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.6159+42.0668 | 22:02:27.65 +42:04:05.5 (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 J330.6159+42.0668,2461119.9486,11.96,0.05,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 J330.6159+42.0668 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:27.65 +42:04:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.90 21:44:52.75 +37:31:14.4
86.81709 -11.94249 galactic Cyg Second-epoch detections are separated by 1.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:52.75 +37:31:14.4 (user input) | T | P | (position from user input) J-Ks=0.658+/-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,2461119.9486,11.90,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:52.75 +37:31:14.4 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1949071109713094272,2461119.9486,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949071109713094272 20260320.4486 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:11.38 +35:33:11.0 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1955341212206396160,2461119.9486,11.88,0.05,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 1955341212206396160 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:09.39 +38:28:30.9 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.11 21:42:24.43 +38:38:04.3
87.19946 -10.78629 galactic Cyg Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:24.43 +38:38:04.3 (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,2461119.9486,12.11,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:24.43 +38:38:04.3 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,12.04,0.05,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
target 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:12.26 +39:12:33.0 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 11.96 21:22:07.72 +36:03:47.0
82.43318 -9.86102 galactic Cyg Second-epoch detections are separated by 3.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.5146+36.0600 | 21:22:04.50 +36:04:02.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G1 (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 J320.5146+36.0600,2461119.9486,11.96,0.05,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 J320.5146+36.0600 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:07.72 +36:03:47.0 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.96,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:28.89 +34:33:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1953796913770434944,2461119.9486,11.93,0.05,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 1953796913770434944 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:06.88 +38:39:19.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.89,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:59:02.42 +37:17:53.3 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.08 21:57:33.98 +41:27:52.4
91.31144 -10.49185 galactic Cyg Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:33.98 +41:27:52.4 (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,2461119.9486,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:33.98 +41:27:52.4 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.06 21:22:56.49 +34:32:30.5
81.44440 -11.04264 galactic Cyg Second-epoch detections are separated by 1.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.7370+34.5401 | 21:22:57.21 +34:31:49.9 (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 J320.7370+34.5401,2461119.9486,12.06,0.05,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
ATO J320.7370+34.5401 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:56.49 +34:32:30.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.02 21:43:16.62 +40:27:47.7
88.55855 -9.52823 galactic Cyg Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:16.62 +40:27:47.7 (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,2461119.9486,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:16.62 +40:27:47.7 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,12.12,0.05,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
V1616 Cyg 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:09.82 +36:39:09.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.05 22:09:15.62 +39:15:32.2
91.74485 -13.59750 galactic Lac Second-epoch detections are separated by 3.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956289747145264384 | 22:09:13.52 +39:15:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.343+/-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 1956289747145264384,2461119.9486,12.05,0.05,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
Gaia DR3 1956289747145264384 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:15.62 +39:15:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.06 21:29:18.98 +40:28:35.8
86.59154 -7.72069 galactic Cyg Second-epoch detections are separated by 0.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.3304+40.4753 | 21:29:18.98 +40:28:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (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
ATO J322.3304+40.4753,2461119.9486,12.06,0.05,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
ATO J322.3304+40.4753 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:18.98 +40:28:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,11.96,0.05,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 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:27.41 +42:00:07.5 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.01 21:38:38.10 +33:58:31.9
83.41108 -13.71563 galactic Cyg Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1947234444258836096 | 21:38:34.61 +33:58:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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
Gaia DR3 1947234444258836096,2461119.9486,12.01,0.05,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 1947234444258836096 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:38.10 +33:58:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1951993886497805696,2461119.9486,12.01,0.05,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 1951993886497805696 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:34.12 +37:11:48.2 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.11 21:52:30.98 +41:28:59.1
90.57634 -9.88222 galactic Cyg Second-epoch detections are separated by 2.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1960357802729664512 | 21:52:34.39 +41:28:42.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.764+/-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
Gaia DR3 1960357802729664512,2461119.9486,12.11,0.05,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 1960357802729664512 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:30.98 +41:28:59.1 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.15 21:53:08.54 +40:33:36.1
90.07263 -10.66983 galactic Cyg Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:08.54 +40:33:36.1 (user input) | T | P | (position from user input) J-Ks=0.925+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.9486,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.4486 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:53:08.54 +40:33:36.1 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.14 21:50:28.68 +37:17:46.8
87.52706 -12.84005 galactic Cyg Second-epoch detections are separated by 1.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.6146+37.2867 | 21:50:28.68 +37:17:46.8 (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+37.2867,2461119.9486,12.14,0.05,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 J327.6146+37.2867 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:28.68 +37:17:46.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.4486 2461119.9486 12.22 21:56:00.35 +37:10:59.6
88.31966 -13.63246 galactic Cyg Second-epoch detections are separated by 2.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9918+37.1927 | 21:56:00.35 +37:10:59.6 (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 J328.9918+37.1927,2461119.9486,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.9918+37.1927 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:00.35 +37:10:59.6 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1953805778581952256,2461119.9486,12.12,0.05,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 1953805778581952256 20260320.4486 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:26.09 +38:30:23.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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 1965294163265869312,2461119.9486,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965294163265869312 20260320.4486 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:09.63 +39:08:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,10.59,0.05,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
IT Peg 20260320.4486 10.59CV 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_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:42.56 +35:43:46.4 ;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_20-20-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2151195+410702,2461119.9486,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2151195+410702 20260320.4486 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:19.77 +41:07:04.8 ;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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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,2461119.9486,10.52,0.05,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
WW Peg 20260320.4486 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/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:37.97 +36:20:34.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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_2026-03-20_05-46-09_20_00sec_-15_00C_LIGHT_0462_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_2026-03-20_05-45-24_20_00sec_-14_90C_LIGHT_0461_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: 2461119.94883558 20.03.2026 10:46:09.394 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
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): 24356
Objects passed selection criteria: 24277
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: 19593.2
Average stars matched: 18276.2 (93.2783 %)
Memory usage VmPeak: 128172 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 05:48:09 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: 2461119.94883558 20.03.2026 10:46:09.394 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 255
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: 72 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): 174189
Objects passed selection criteria: 173734
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 139805
Average stars matched: 129543 (92.6598 %)
Memory usage VmPeak: 2055056 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 05:51:10 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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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: 2461119.94831274
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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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 21:48:58.811 +37:59:41.07
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:48:48.775 +38:01:54.18
Second-epoch image center 21:48:57.277 +37:59:37.08
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:48:58.811 +37:59:41.07
Second-epoch second image center 21:48:57.277 +37:59:37.08
Angular distance between the image centers 0.00516 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.bRMI5hh9wK
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.dIO4vQDVdb
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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits &> /tmp/tmp.drBSdwEupA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits &> /tmp/tmp.fX3Ds1dWAC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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 7 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
2.6 pix fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
2.7 pix fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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
14.6 mag. fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
14.6 mag. fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.8 (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.bRMI5hh9wK (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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.dIO4vQDVdb (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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.drBSdwEupA (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1244, passed=18904
Got 18904 stars (including 17639 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat
util/solve_plate_with_UCAC5 got 18904 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (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 0.010437 (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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 956 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.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.fX3Ds1dWAC (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1195, passed=19126
Got 19126 stars (including 17911 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat
util/solve_plate_with_UCAC5 got 19126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (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 0.010437 (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 954 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: 0.59"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out34524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34767.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): 3s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32288_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 32288_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:51:19.35 +36:49:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32493_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 32493_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:48:31.50 +42:05:28.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33571_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 33571_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:49:56.74 +40:56:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33665_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 33665_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:34:49.08 +38:30:13.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34524_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 34524_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:50:15.68 +35:39:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.939 1949260878546849536 327.56564057233 +35.65960337615 11.4772 10.4690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34767_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 34767_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:24:56.22 +37:11:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 3.553 1963793261174257152 321.23536600714 +37.18820597676 12.2607 11.8353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10857_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 10857_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
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 ####
22:12:51.16 +39:09:59.2
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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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 21:48:58.811 +37:59:41.07
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:48:48.775 +38:01:54.18
Second-epoch image center 21:48:57.277 +37:59:37.08
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:48:58.811 +37:59:41.07
Second-epoch second image center 21:48:57.277 +37:59:37.08
Angular distance between the image centers 0.00516 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.PxGLDNm0HQ
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.Ubhj7GopN3
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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits &> /tmp/tmp.YZ6xqa5wIk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits &> /tmp/tmp.2zl2kE2JuZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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 203 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
2.5 pix fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
2.6 pix fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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
12.9 mag. fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
12.8 mag. fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.2 (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.PxGLDNm0HQ (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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.Ubhj7GopN3 (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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.YZ6xqa5wIk (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=13529, passed=122547
Got 122547 stars (including 108882 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat
util/solve_plate_with_UCAC5 got 122547 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (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 0.010437 (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: 0.59"
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 962 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: 0.62"
Excluding outliers - 960 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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.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.2zl2kE2JuZ (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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=12552, passed=117350
Got 117350 stars (including 104678 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat
util/solve_plate_with_UCAC5 got 117350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (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 0.010437 (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: 0.59"
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 962 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: 0.62"
Excluding outliers - 960 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_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/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_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-45-24_20.00sec_-14.90C_LIGHT_0461.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.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_2026-03-20_CI_Cyg-07-Q2b1x1_054647_TTUQ2b1x1_32404_d68LkoiP/wcs_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462.fits
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out242692.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__out226838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out231341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out233909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out242980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out243896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43101.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 116s
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: 54s
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Considering the candidate 226838_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226838_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226842_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226842_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226856_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226856_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226863_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226863_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226869_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226869_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226875_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226875_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226877_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226877_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226879_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226879_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226884_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226884_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226885_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226885_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226890_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226890_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226892_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226892_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226893_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226893_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226895_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226895_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226896_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226896_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226906_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226906_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226907_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226907_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226908_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226908_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226909_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226909_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226911_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226911_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 226912_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 226912_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 226917_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 226917_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 229332_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 229332_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 231341_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 231341_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 231384_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 231384_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:23:40.19 +37:20:46.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 231505_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 231505_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 232061_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 232061_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 233624_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 233624_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 233909_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 233909_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 234222_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 234222_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 234828_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 234828_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 234832_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 234832_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234935_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 234935_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 235007_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 235007_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 235464_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 235464_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 235516_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 235516_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 235518_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 235518_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 235975_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 235975_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236023_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 236023_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 236066_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 236066_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 236359_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 236359_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236543_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 236543_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 236707_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 236707_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 236767_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 236767_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:48:22.56 +38:39:59.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236924_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 236924_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236935_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 236935_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237068_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 237068_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 237137_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 237137_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237389_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 237389_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 237420_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 237420_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 237774_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 237774_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237788_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 237788_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 237845_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 237845_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 237877_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 237877_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 238051_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 238051_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238109_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238109_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 238117_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 238117_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238232_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238232_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 238287_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 238287_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238409_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238409_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 238470_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 238470_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238652_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238652_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238671_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238671_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 238694_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238694_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 238740_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238740_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238752_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 238752_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 238774_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238774_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:51:45.86 +41:39:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 238883_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 238883_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239029_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 239029_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239143_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 239143_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239263_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 239263_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 239438_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 239438_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239724_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 239724_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239742_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 239742_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239773_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 239773_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240169_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 240169_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240171_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 240171_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240221_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 240221_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240357_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 240357_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 240364_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 240364_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 240473_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 240473_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240562_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 240562_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240774_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 240774_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 240934_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 240934_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240963_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 240963_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241003_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 241003_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 241036_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241036_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241058_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241058_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241066_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 241066_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 241144_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 241144_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 241254_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 241254_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 241297_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241297_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241309_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241309_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241399_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241399_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241496_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241496_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241651_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241651_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241699_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241699_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241719_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241719_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241860_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 241860_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 241878_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 241878_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 242009_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242009_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242137_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242137_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242240_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242240_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242299_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242299_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242333_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242333_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242344_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242344_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242401_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242401_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 242413_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242413_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 242515_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242515_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:47:58.59 +36:34:48.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242581_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242581_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242609_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242609_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 242614_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242614_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 242692_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242692_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:51:29.30 +38:43:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.614 1953105905067981952 327.87158794961 +38.71955905257 11.8663 9.9472 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 242736_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242736_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242743_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242743_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242783_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242783_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 242853_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242853_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 242927_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 242927_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 242980_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 242980_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243048_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 243048_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 243101_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 243101_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 243125_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 243125_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243303_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 243303_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243330_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 243330_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243350_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 243350_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243425_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 243425_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243688_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 243688_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243846_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 243846_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 243896_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 243896_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 243927_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 243927_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 244059_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244059_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 244199_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244199_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 244218_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244218_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244239_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244239_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 244333_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244333_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 244440_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244440_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244495_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 244495_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 244522_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 244522_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 244586_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244586_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 244624_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 244624_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 244656_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 244656_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 244969_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 244969_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 245079_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 245079_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 245199_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 245199_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 245236_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 245236_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245459_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 245459_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 245596_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 245596_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 245682_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 245682_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 245689_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 245689_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 245723_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 245723_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 245857_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 245857_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 245981_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 245981_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 246190_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 246190_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 246334_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 246334_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 246363_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 246363_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 246449_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 246449_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 246507_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 246507_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 246640_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 246640_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 246899_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 246899_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 246900_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 246900_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 246973_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 246973_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 247515_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 247515_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 247771_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 247771_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 247807_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 247807_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 248072_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248072_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 248120_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248120_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 248165_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248165_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 248196_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248196_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 248214_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248214_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 248381_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248381_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 248497_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248497_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 248528_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248528_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 248599_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248599_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 248662_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248662_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 248799_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248799_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 248981_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 248981_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 249557_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 249557_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 249598_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 249598_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 249757_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 249757_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 249946_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 249946_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 249986_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 249986_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 250046_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250046_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 250094_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250094_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 250097_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250097_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 250167_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250167_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 250220_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250220_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 250264_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250264_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 250288_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250288_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 250323_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 250323_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 250378_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250378_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 250388_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250388_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 250407_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250407_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 250423_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 250423_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 219051_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 219051_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 43101_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 43101_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 47611_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 47611_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:49:56.76 +40:56:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76443_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 76443_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 22:12:51.15 +39:09:59.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 129504_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 129504_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:51:19.36 +36:49:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138402_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
Preparing report for the candidate 138402_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
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Considering the candidate 100239_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 100239_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 44711_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 44711_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 24612_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 24612_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
**** FOUND 21:48:31.50 +42:05:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97151_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462
The candidate 97151_fd_Cyg-07-Q2b1x1_2026-03-20_05-46-09_20.00sec_-15.00C_LIGHT_0462 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 20s
make_report_in_HTML.sh TOTAL: 190s
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 ####
22:12:51.16 +39:09:59.2
21:56:37.97 +36:20:34.5
22:03:42.56 +35:43:46.4
21:36:51.86 +34:54:48.4
21:31:59.67 +39:17:14.9
21:27:27.09 +41:06:11.3
22:12:40.47 +37:26:57.5
21:23:49.98 +35:00:32.1
21:32:27.33 +38:28:56.2
22:04:57.05 +36:16:51.2
21:20:00.07 +38:24:37.6
21:48:12.40 +41:41:12.8
21:45:29.64 +42:12:24.5
21:37:53.92 +40:49:54.0
21:20:51.21 +38:55:12.7
21:34:11.06 +35:48:32.9
21:41:48.75 +35:04:55.2
21:20:26.95 +35:31:38.5
21:19:57.28 +39:52:27.1
21:41:19.36 +37:02:33.7
21:22:26.02 +37:11:04.3
21:40:56.21 +41:13:23.5
21:18:16.70 +37:55:33.7
21:46:27.04 +42:00:02.8
21:47:57.29 +36:35:34.2
21:31:14.69 +39:26:58.9
21:35:04.81 +40:51:23.3
21:52:09.49 +38:58:10.0
21:58:48.39 +41:41:43.8
22:13:14.50 +41:47:43.5
21:33:36.29 +38:32:50.2
21:42:55.22 +41:08:31.8
22:12:58.61 +38:26:20.2
21:32:54.31 +35:30:11.4
21:38:32.00 +39:29:21.8
21:48:53.57 +40:38:12.5
21:42:50.08 +38:10:46.2
21:42:06.12 +36:50:54.8
21:58:07.66 +38:56:42.5
21:24:18.17 +34:35:15.9
21:55:05.16 +34:46:31.1
22:07:50.34 +40:07:29.1
21:41:14.62 +41:17:58.5
21:57:28.46 +41:27:31.9
22:05:09.89 +37:27:59.8
22:11:22.94 +39:44:15.4
21:50:52.28 +39:37:42.5
21:59:27.29 +38:47:17.4
21:35:30.50 +34:46:53.1
21:39:39.44 +39:57:29.0
22:09:46.33 +41:39:57.4
22:00:54.51 +41:16:15.5
22:02:40.05 +38:06:48.8
22:01:13.37 +38:32:59.5
21:46:21.84 +39:50:09.2
21:39:20.67 +35:38:19.5
22:03:59.93 +39:46:40.3
22:13:05.26 +41:48:42.1
21:31:09.91 +36:52:32.6
21:41:13.46 +41:18:24.1
21:36:04.27 +41:56:43.7
21:38:02.70 +39:00:12.2
21:57:20.63 +40:57:00.9
21:41:14.17 +41:15:47.8
21:38:09.12 +38:56:14.9
21:44:17.21 +39:14:05.5
21:20:02.44 +34:06:12.1
21:44:49.63 +36:56:56.7
21:49:54.51 +34:54:44.0
21:23:15.79 +35:12:51.0
22:02:27.65 +42:04:05.5
21:44:52.75 +37:31:14.4
21:50:11.38 +35:33:11.0
22:14:09.39 +38:28:30.9
21:42:24.43 +38:38:04.3
21:35:12.26 +39:12:33.0
21:22:07.72 +36:03:47.0
21:31:28.89 +34:33:29.7
21:35:06.88 +38:39:19.2
21:59:02.42 +37:17:53.3
21:57:33.98 +41:27:52.4
21:22:56.49 +34:32:30.5
21:43:16.62 +40:27:47.7
21:41:09.82 +36:39:09.2
22:09:15.62 +39:15:32.2
21:29:18.98 +40:28:35.8
21:55:27.41 +42:00:07.5
21:38:38.10 +33:58:31.9
21:36:34.12 +37:11:48.2
21:52:30.98 +41:28:59.1
21:53:08.54 +40:33:36.1
21:50:28.68 +37:17:46.8
21:56:00.35 +37:10:59.6
21:34:26.09 +38:30:23.8
21:24:09.63 +39:08:30.1
21:51:19.77 +41:07:04.8
########### 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 ####
22:12:51.16 +39:09:59.2
21:36:51.86 +34:54:48.4
21:31:59.67 +39:17:14.9
21:27:27.09 +41:06:11.3
22:12:40.47 +37:26:57.5
21:23:49.98 +35:00:32.1
21:32:27.33 +38:28:56.2
22:04:57.05 +36:16:51.2
21:20:00.07 +38:24:37.6
21:48:12.40 +41:41:12.8
21:45:29.64 +42:12:24.5
21:37:53.92 +40:49:54.0
21:20:51.21 +38:55:12.7
21:34:11.06 +35:48:32.9
21:41:48.75 +35:04:55.2
21:20:26.95 +35:31:38.5
21:19:57.28 +39:52:27.1
21:41:19.36 +37:02:33.7
21:22:26.02 +37:11:04.3
21:40:56.21 +41:13:23.5
21:18:16.70 +37:55:33.7
21:46:27.04 +42:00:02.8
21:47:57.29 +36:35:34.2
21:31:14.69 +39:26:58.9
21:35:04.81 +40:51:23.3
21:52:09.49 +38:58:10.0
21:58:48.39 +41:41:43.8
22:13:14.50 +41:47:43.5
21:33:36.29 +38:32:50.2
21:42:55.22 +41:08:31.8
22:12:58.61 +38:26:20.2
21:32:54.31 +35:30:11.4
21:38:32.00 +39:29:21.8
21:48:53.57 +40:38:12.5
21:42:50.08 +38:10:46.2
21:42:06.12 +36:50:54.8
21:58:07.66 +38:56:42.5
21:24:18.17 +34:35:15.9
21:55:05.16 +34:46:31.1
22:07:50.34 +40:07:29.1
21:41:14.62 +41:17:58.5
21:57:28.46 +41:27:31.9
22:05:09.89 +37:27:59.8
22:11:22.94 +39:44:15.4
21:50:52.28 +39:37:42.5
21:59:27.29 +38:47:17.4
21:35:30.50 +34:46:53.1
21:39:39.44 +39:57:29.0
22:09:46.33 +41:39:57.4
22:00:54.51 +41:16:15.5
22:02:40.05 +38:06:48.8
22:01:13.37 +38:32:59.5
21:46:21.84 +39:50:09.2
21:39:20.67 +35:38:19.5
22:03:59.93 +39:46:40.3
22:13:05.26 +41:48:42.1
21:31:09.91 +36:52:32.6
21:41:13.46 +41:18:24.1
21:36:04.27 +41:56:43.7
21:38:02.70 +39:00:12.2
21:57:20.63 +40:57:00.9
21:41:14.17 +41:15:47.8
21:38:09.12 +38:56:14.9
21:44:17.21 +39:14:05.5
21:20:02.44 +34:06:12.1
21:44:49.63 +36:56:56.7
21:49:54.51 +34:54:44.0
21:23:15.79 +35:12:51.0
22:02:27.65 +42:04:05.5
21:44:52.75 +37:31:14.4
21:50:11.38 +35:33:11.0
22:14:09.39 +38:28:30.9
21:42:24.43 +38:38:04.3
21:35:12.26 +39:12:33.0
21:22:07.72 +36:03:47.0
21:31:28.89 +34:33:29.7
21:35:06.88 +38:39:19.2
21:59:02.42 +37:17:53.3
21:57:33.98 +41:27:52.4
21:22:56.49 +34:32:30.5
21:43:16.62 +40:27:47.7
21:41:09.82 +36:39:09.2
22:09:15.62 +39:15:32.2
21:29:18.98 +40:28:35.8
21:55:27.41 +42:00:07.5
21:38:38.10 +33:58:31.9
21:36:34.12 +37:11:48.2
21:52:30.98 +41:28:59.1
21:53:08.54 +40:33:36.1
21:50:28.68 +37:17:46.8
21:56:00.35 +37:10:59.6
21:34:26.09 +38:30:23.8
21:24:09.63 +39:08:30.1
22:03:42.56 +35:43:46.4
21:51:19.77 +41:07:04.8
21:56:37.97 +36:20:34.5
###################################################################################
22:12:51.16 +39:09:59.2 -- not an asteroid (will add it to exclusion list)
21:36:51.86 +34:54:48.4 -- not an asteroid (will add it to exclusion list)
21:31:59.67 +39:17:14.9 -- not an asteroid (will add it to exclusion list)
21:27:27.09 +41:06:11.3 -- not an asteroid (will add it to exclusion list)
22:12:40.47 +37:26:57.5 -- not an asteroid (will add it to exclusion list)
21:23:49.98 +35:00:32.1 -- not an asteroid (will add it to exclusion list)
21:32:27.33 +38:28:56.2 -- not an asteroid (will add it to exclusion list)
22:04:57.05 +36:16:51.2 -- not an asteroid (will add it to exclusion list)
21:20:00.07 +38:24:37.6 -- not an asteroid (will add it to exclusion list)
21:48:12.40 +41:41:12.8 -- not an asteroid (will add it to exclusion list)
21:45:29.64 +42:12:24.5 -- not an asteroid (will add it to exclusion list)
21:37:53.92 +40:49:54.0 -- not an asteroid (will add it to exclusion list)
21:20:51.21 +38:55:12.7 -- not an asteroid (will add it to exclusion list)
21:34:11.06 +35:48:32.9 -- not an asteroid (will add it to exclusion list)
21:41:48.75 +35:04:55.2 -- not an asteroid (will add it to exclusion list)
21:20:26.95 +35:31:38.5 -- not an asteroid (will add it to exclusion list)
21:19:57.28 +39:52:27.1 -- not an asteroid (will add it to exclusion list)
21:41:19.36 +37:02:33.7 -- not an asteroid (will add it to exclusion list)
21:22:26.02 +37:11:04.3 -- not an asteroid (will add it to exclusion list)
21:40:56.21 +41:13:23.5 -- not an asteroid (will add it to exclusion list)
21:18:16.70 +37:55:33.7 -- not an asteroid (will add it to exclusion list)
21:46:27.04 +42:00:02.8 -- not an asteroid (will add it to exclusion list)
21:47:57.29 +36:35:34.2 -- not an asteroid (will add it to exclusion list)
21:31:14.69 +39:26:58.9 -- not an asteroid (will add it to exclusion list)
21:35:04.81 +40:51:23.3 -- not an asteroid (will add it to exclusion list)
21:52:09.49 +38:58:10.0 -- not an asteroid (will add it to exclusion list)
21:58:48.39 +41:41:43.8 -- not an asteroid (will add it to exclusion list)
22:13:14.50 +41:47:43.5 -- not an asteroid (will add it to exclusion list)
21:33:36.29 +38:32:50.2 -- not an asteroid (will add it to exclusion list)
21:42:55.22 +41:08:31.8 -- not an asteroid (will add it to exclusion list)
22:12:58.61 +38:26:20.2 -- not an asteroid (will add it to exclusion list)
21:32:54.31 +35:30:11.4 -- not an asteroid (will add it to exclusion list)
21:38:32.00 +39:29:21.8 -- not an asteroid (will add it to exclusion list)
21:48:53.57 +40:38:12.5 -- not an asteroid (will add it to exclusion list)
21:42:50.08 +38:10:46.2 -- not an asteroid (will add it to exclusion list)
21:42:06.12 +36:50:54.8 -- not an asteroid (will add it to exclusion list)
21:58:07.66 +38:56:42.5 -- not an asteroid (will add it to exclusion list)
21:24:18.17 +34:35:15.9 -- not an asteroid (will add it to exclusion list)
21:55:05.16 +34:46:31.1 -- not an asteroid (will add it to exclusion list)
22:07:50.34 +40:07:29.1 -- not an asteroid (will add it to exclusion list)
21:41:14.62 +41:17:58.5 -- not an asteroid (will add it to exclusion list)
21:57:28.46 +41:27:31.9 -- not an asteroid (will add it to exclusion list)
22:05:09.89 +37:27:59.8 -- not an asteroid (will add it to exclusion list)
22:11:22.94 +39:44:15.4 -- not an asteroid (will add it to exclusion list)
21:50:52.28 +39:37:42.5 -- not an asteroid (will add it to exclusion list)
21:59:27.29 +38:47:17.4 -- not an asteroid (will add it to exclusion list)
21:35:30.50 +34:46:53.1 -- not an asteroid (will add it to exclusion list)
21:39:39.44 +39:57:29.0 -- not an asteroid (will add it to exclusion list)
22:09:46.33 +41:39:57.4 -- not an asteroid (will add it to exclusion list)
22:00:54.51 +41:16:15.5 -- not an asteroid (will add it to exclusion list)
22:02:40.05 +38:06:48.8 -- not an asteroid (will add it to exclusion list)
22:01:13.37 +38:32:59.5 -- not an asteroid (will add it to exclusion list)
21:46:21.84 +39:50:09.2 -- not an asteroid (will add it to exclusion list)
21:39:20.67 +35:38:19.5 -- not an asteroid (will add it to exclusion list)
22:03:59.93 +39:46:40.3 -- not an asteroid (will add it to exclusion list)
22:13:05.26 +41:48:42.1 -- not an asteroid (will add it to exclusion list)
21:31:09.91 +36:52:32.6 -- not an asteroid (will add it to exclusion list)
21:41:13.46 +41:18:24.1 -- not an asteroid (will add it to exclusion list)
21:36:04.27 +41:56:43.7 -- not an asteroid (will add it to exclusion list)
21:38:02.70 +39:00:12.2 -- not an asteroid (will add it to exclusion list)
21:57:20.63 +40:57:00.9 -- not an asteroid (will add it to exclusion list)
21:41:14.17 +41:15:47.8 -- not an asteroid (will add it to exclusion list)
21:38:09.12 +38:56:14.9 -- not an asteroid (will add it to exclusion list)
21:44:17.21 +39:14:05.5 -- not an asteroid (will add it to exclusion list)
21:20:02.44 +34:06:12.1 -- not an asteroid (will add it to exclusion list)
21:44:49.63 +36:56:56.7 -- not an asteroid (will add it to exclusion list)
21:49:54.51 +34:54:44.0 -- not an asteroid (will add it to exclusion list)
21:23:15.79 +35:12:51.0 -- not an asteroid (will add it to exclusion list)
22:02:27.65 +42:04:05.5 -- not an asteroid (will add it to exclusion list)
21:44:52.75 +37:31:14.4 -- not an asteroid (will add it to exclusion list)
21:50:11.38 +35:33:11.0 -- not an asteroid (will add it to exclusion list)
22:14:09.39 +38:28:30.9 -- not an asteroid (will add it to exclusion list)
21:42:24.43 +38:38:04.3 -- not an asteroid (will add it to exclusion list)
21:35:12.26 +39:12:33.0 -- not an asteroid (will add it to exclusion list)
21:22:07.72 +36:03:47.0 -- not an asteroid (will add it to exclusion list)
21:31:28.89 +34:33:29.7 -- not an asteroid (will add it to exclusion list)
21:35:06.88 +38:39:19.2 -- not an asteroid (will add it to exclusion list)
21:59:02.42 +37:17:53.3 -- not an asteroid (will add it to exclusion list)
21:57:33.98 +41:27:52.4 -- not an asteroid (will add it to exclusion list)
21:22:56.49 +34:32:30.5 -- not an asteroid (will add it to exclusion list)
21:43:16.62 +40:27:47.7 -- not an asteroid (will add it to exclusion list)
21:41:09.82 +36:39:09.2 -- not an asteroid (will add it to exclusion list)
22:09:15.62 +39:15:32.2 -- not an asteroid (will add it to exclusion list)
21:29:18.98 +40:28:35.8 -- not an asteroid (will add it to exclusion list)
21:55:27.41 +42:00:07.5 -- not an asteroid (will add it to exclusion list)
21:38:38.10 +33:58:31.9 -- not an asteroid (will add it to exclusion list)
21:36:34.12 +37:11:48.2 -- not an asteroid (will add it to exclusion list)
21:52:30.98 +41:28:59.1 -- not an asteroid (will add it to exclusion list)
21:53:08.54 +40:33:36.1 -- not an asteroid (will add it to exclusion list)
21:50:28.68 +37:17:46.8 -- not an asteroid (will add it to exclusion list)
21:56:00.35 +37:10:59.6 -- not an asteroid (will add it to exclusion list)
21:34:26.09 +38:30:23.8 -- not an asteroid (will add it to exclusion list)
21:24:09.63 +39:08:30.1 -- not an asteroid (will add it to exclusion list)
22:03:42.56 +35:43:46.4 -- not an asteroid (will add it to exclusion list)
21:51:19.77 +41:07:04.8 -- not an asteroid (will add it to exclusion list)
21:56:37.97 +36:20:34.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:18:16.70 +37:55:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:57.28 +39:52:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:00.07 +38:24:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:02.44 +34:06:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:26.95 +35:31:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:51.21 +38:55:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:07.72 +36:03:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:26.02 +37:11:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:56.49 +34:32:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:15.79 +35:12:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:49.98 +35:00:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:09.63 +39:08:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:18.17 +34:35:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:27.09 +41:06:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:18.98 +40:28:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:09.91 +36:52:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.69 +39:26:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.89 +34:33:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:59.67 +39:17:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:27.33 +38:28:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:54.31 +35:30:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:36.29 +38:32:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:11.06 +35:48:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:26.09 +38:30:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:04.81 +40:51:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:06.88 +38:39:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:12.26 +39:12:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:30.50 +34:46:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:04.27 +41:56:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:34.12 +37:11:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:51.86 +34:54:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:53.92 +40:49:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:02.70 +39:00:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:09.12 +38:56:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:32.00 +39:29:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:38.10 +33:58:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:20.67 +35:38:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:39.44 +39:57:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.21 +41:13:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:09.82 +36:39:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:13.46 +41:18:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:14.17 +41:15:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:14.62 +41:17:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:19.36 +37:02:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:48.75 +35:04:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:06.12 +36:50:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:24.43 +38:38:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:50.08 +38:10:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:55.22 +41:08:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:16.62 +40:27:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:17.21 +39:14:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:49.63 +36:56:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:52.75 +37:31:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:29.64 +42:12:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:21.84 +39:50:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:27.04 +42:00:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:57.29 +36:35:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:12.40 +41:41:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:53.57 +40:38:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:54.51 +34:54:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:11.38 +35:33:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:28.68 +37:17:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:52.28 +39:37:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:19.77 +41:07:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:09.49 +38:58:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:30.98 +41:28:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:08.54 +40:33:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:05.16 +34:46:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:27.41 +42:00:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.35 +37:10:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:37.97 +36:20:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:20.63 +40:57:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:28.46 +41:27:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:33.98 +41:27:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:07.66 +38:56:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:48.39 +41:41:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:02.42 +37:17:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:27.29 +38:47:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:54.51 +41:16:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:13.37 +38:32:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:27.65 +42:04:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:40.05 +38:06:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:42.56 +35:43:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:59.93 +39:46:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:57.05 +36:16:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:09.89 +37:27:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:50.34 +40:07:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:15.62 +39:15:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:46.33 +41:39:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:22.94 +39:44:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:40.47 +37:26:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:51.16 +39:09:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:58.61 +38:26:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:05.26 +41:48:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:14.50 +41:47:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:09.39 +38:28:30.9 -- 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)
21:18:16.70 +37:55:33.7 -- a known variable star
21:19:57.28 +39:52:27.1 -- not a known variable star
21:20:00.07 +38:24:37.6 -- a known variable star
21:20:02.44 +34:06:12.1 -- not a known variable star
21:20:26.95 +35:31:38.5 -- not a known variable star
21:20:51.21 +38:55:12.7 -- not a known variable star
21:22:07.72 +36:03:47.0 -- not a known variable star
21:22:26.02 +37:11:04.3 -- not a known variable star
21:22:56.49 +34:32:30.5 -- not a known variable star
21:23:15.79 +35:12:51.0 -- not a known variable star
21:23:49.98 +35:00:32.1 -- not a known variable star
21:24:09.63 +39:08:30.1 -- a known variable star
21:24:18.17 +34:35:15.9 -- not a known variable star
21:27:27.09 +41:06:11.3 -- not a known variable star
21:29:18.98 +40:28:35.8 -- not a known variable star
21:31:09.91 +36:52:32.6 -- not a known variable star
21:31:14.69 +39:26:58.9 -- a known variable star
21:31:28.89 +34:33:29.7 -- not a known variable star
21:31:59.67 +39:17:14.9 -- not a known variable star
21:32:27.33 +38:28:56.2 -- not a known variable star
21:32:54.31 +35:30:11.4 -- not a known variable star
21:33:36.29 +38:32:50.2 -- not a known variable star
21:34:11.06 +35:48:32.9 -- not a known variable star
21:34:26.09 +38:30:23.8 -- a known variable star
21:35:04.81 +40:51:23.3 -- a known variable star
21:35:06.88 +38:39:19.2 -- a known variable star
21:35:12.26 +39:12:33.0 -- not a known variable star
21:35:30.50 +34:46:53.1 -- not a known variable star
21:36:04.27 +41:56:43.7 -- not a known variable star
21:36:34.12 +37:11:48.2 -- a known variable star
21:36:51.86 +34:54:48.4 -- not a known variable star
21:37:53.92 +40:49:54.0 -- not a known variable star
21:38:02.70 +39:00:12.2 -- a known variable star
21:38:09.12 +38:56:14.9 -- not a known variable star
21:38:32.00 +39:29:21.8 -- not a known variable star
21:38:38.10 +33:58:31.9 -- not a known variable star
21:39:20.67 +35:38:19.5 -- not a known variable star
21:39:39.44 +39:57:29.0 -- not a known variable star
21:40:56.21 +41:13:23.5 -- not a known variable star
21:41:09.82 +36:39:09.2 -- a known variable star
21:41:13.46 +41:18:24.1 -- not a known variable star
21:41:14.17 +41:15:47.8 -- not a known variable star
21:41:14.62 +41:17:58.5 -- a known variable star
21:41:19.36 +37:02:33.7 -- not a known variable star
21:41:48.75 +35:04:55.2 -- not a known variable star
21:42:06.12 +36:50:54.8 -- not a known variable star
21:42:24.43 +38:38:04.3 -- not a known variable star
21:42:50.08 +38:10:46.2 -- not a known variable star
21:42:55.22 +41:08:31.8 -- not a known variable star
21:43:16.62 +40:27:47.7 -- not a known variable star
21:44:17.21 +39:14:05.5 -- not a known variable star
21:44:49.63 +36:56:56.7 -- not a known variable star
21:44:52.75 +37:31:14.4 -- not a known variable star
21:45:29.64 +42:12:24.5 -- a known variable star
21:46:21.84 +39:50:09.2 -- not a known variable star
21:46:27.04 +42:00:02.8 -- not a known variable star
21:47:57.29 +36:35:34.2 -- not a known variable star
21:48:12.40 +41:41:12.8 -- not a known variable star
21:48:53.57 +40:38:12.5 -- not a known variable star
21:49:54.51 +34:54:44.0 -- not a known variable star
21:50:11.38 +35:33:11.0 -- a known variable star
21:50:28.68 +37:17:46.8 -- not a known variable star
21:50:52.28 +39:37:42.5 -- not a known variable star
21:51:19.77 +41:07:04.8 -- a known variable star
21:52:09.49 +38:58:10.0 -- not a known variable star
21:52:30.98 +41:28:59.1 -- not a known variable star
21:53:08.54 +40:33:36.1 -- not a known variable star
21:55:05.16 +34:46:31.1 -- not a known variable star
21:55:27.41 +42:00:07.5 -- not a known variable star
21:56:00.35 +37:10:59.6 -- not a known variable star
21:56:37.97 +36:20:34.5 -- a known variable star
21:57:20.63 +40:57:00.9 -- not a known variable star
21:57:28.46 +41:27:31.9 -- not a known variable star
21:57:33.98 +41:27:52.4 -- not a known variable star
21:58:07.66 +38:56:42.5 -- not a known variable star
21:58:48.39 +41:41:43.8 -- not a known variable star
21:59:02.42 +37:17:53.3 -- not a known variable star
21:59:27.29 +38:47:17.4 -- not a known variable star
22:00:54.51 +41:16:15.5 -- not a known variable star
22:01:13.37 +38:32:59.5 -- not a known variable star
22:02:27.65 +42:04:05.5 -- not a known variable star
22:02:40.05 +38:06:48.8 -- not a known variable star
22:03:42.56 +35:43:46.4 -- a known variable star
22:03:59.93 +39:46:40.3 -- not a known variable star
22:04:57.05 +36:16:51.2 -- not a known variable star
22:05:09.89 +37:27:59.8 -- not a known variable star
22:07:50.34 +40:07:29.1 -- not a known variable star
22:09:15.62 +39:15:32.2 -- not a known variable star
22:09:46.33 +41:39:57.4 -- not a known variable star
22:11:22.94 +39:44:15.4 -- not a known variable star
22:12:40.47 +37:26:57.5 -- not a known variable star
22:12:51.16 +39:09:59.2 -- a known variable star
22:12:58.61 +38:26:20.2 -- a known variable star
22:13:05.26 +41:48:42.1 -- not a known variable star
22:13:14.50 +41:47:43.5 -- not a known variable star
22:14:09.39 +38:28:30.9 -- a known variable star
Found 77 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
96 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 96 (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)2461119.94831274 -observatory 500
22:37:30.46 -07:31:18.4 Mercury (1.1mag)
01:04:03.93 +05:52:16.4 Venus (-3.9mag)
23:01:33.37 -07:24:24.6 Mars (1.2mag)
07:04:41.34 +22:58:06.0 Jupiter (-2.3mag)
00:17:05.78 -00:27:48.5 Saturn (0.9mag)
03:42:51.15 +19:31:35.7 Uranus (5.8mag)
00:07:12.79 -00:38:31.9 Neptune (7.8mag)
20:31:57.36 -22:53:52.2 Pluto (14.5mag)
01:00:21.21 +10:01:49.8 Moon (-8.5mag)
-rw-r--r-- 1 apache apache 361 Mar 20 05:48 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461119.94831274:
07:04:38.54 +22:58:13.8 Io (5.6mag)
07:04:35.81 +22:58:13.2 Europa (5.7mag)
07:04:26.32 +22:58:27.8 Ganymede (5.2mag)
07:04:09.70 +22:58:57.3 Callisto (6.4mag)
07:08:42.75 +23:00:02.2 Himalia (15.2mag)
07:04:42.63 +22:58:05.9 Thebe (16.0mag)
07:08:16.93 +23:23:04.2 Elara (17.2mag)
07:01:47.20 +23:52:04.5 Pasiphae (17.2mag)
07:13:29.22 +22:52:27.2 Carme (18.3mag)
00:16:58.33 -00:27:39.9 Titan (8.8mag)
00:17:07.17 -00:27:46.0 Rhea (10.1mag)
00:17:35.95 -00:25:48.6 Iapetus (11.5mag)
00:17:20.34 -00:27:56.0 Hyperion (14.8mag)
00:19:00.21 -00:16:29.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 20 05:48 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.94831274:
12:45:16.07 +09:26:18.8 JWST
03:41:20.76 -51:39:14.0 Chandra
18:50:17.32 -02:45:41.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 20 05:48 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.94831274 -observatory 500
18:34:56.26 -27:26:14.7 14.1mag P/2010 H2 (Vales)
04:50:54.65 -71:03:54.1 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:42.12 +31:17:46.2 17.0mag C/2017 K2 (PANSTARRS)
17:29:32.49 +07:20:19.3 17.6mag C/2021 G2 (ATLAS)
23:01:20.49 +28:25:32.4 16.9mag C/2022 E2 (ATLAS)
03:59:55.69 +25:16:42.8 15.7mag C/2022 N2 (PANSTARRS)
09:01:56.71 +31:25:36.2 16.0mag C/2022 QE78 (ATLAS)
08:30:14.67 -03:14:45.4 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.78 +16:14:40.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:24.59 -11:51:01.8 17.6mag P/2023 B1 (PANSTARRS)
09:24:59.71 -16:25:30.3 17.4mag C/2023 F3 (ATLAS)
21:20:51.94 +61:40:44.3 17.4mag C/2023 H5 (Lemmon)
19:33:20.14 -03:31:07.6 14.5mag C/2023 R1 (PANSTARRS)
21:35:52.28 +82:48:20.5 17.7mag C/2023 X2 (Lemmon)
06:15:35.55 +63:47:36.9 16.8mag C/2024 A1 (ATLAS)
04:04:38.05 +04:47:26.9 9.1mag C/2024 E1 (Wierzchos)
11:23:05.78 +02:37:17.2 18.0mag C/2024 G2 (ATLAS)
16:32:27.83 +02:04:41.6 17.5mag C/2024 G6 (ATLAS)
20:09:45.67 +08:38:19.1 14.9mag C/2024 J3 (ATLAS)
03:04:17.24 -26:45:02.0 16.5mag C/2024 T5 (ATLAS)
04:57:13.38 +52:46:57.0 17.6mag C/2025 J1 (Borisov)
15:15:15.03 +16:43:12.8 14.4mag C/2025 L1 (ATLAS)
02:47:50.54 -22:30:30.4 17.6mag C/2025 Q3 (ATLAS)
22:32:33.01 +18:58:40.5 12.5mag C/2025 R3 (PANSTARRS)
13:05:16.58 +01:16:31.6 17.6mag C/2025 Y1 (ATLAS)
02:11:09.02 -06:41:38.1 14.2mag C/2026 A1 (MAPS)
22:37:03.08 +30:52:39.0 13.7mag C/2026 B2 (Sun-Gao)
17:50:59.04 -10:51:24.8 13.3mag 10P/Tempel
15:27:02.18 +05:09:52.8 11.7mag 24P/Schaumasse
11:12:13.83 -02:30:08.3 15.6mag 29P/Schwassmann-Wachmann
17:43:05.23 -10:39:59.0 17.3mag 40P/Vaisala
10:45:26.73 -06:37:22.4 16.4mag 43P/Wolf-Harrington
01:08:07.75 +12:49:26.4 17.0mag 47P/Ashbrook-Jackson
06:27:51.56 +42:27:30.7 17.1mag 63P/Wild
22:53:25.31 -14:48:55.1 15.7mag 65P/Gunn
02:57:11.45 +11:05:33.7 15.9mag 76P/West-Kohoutek-Ikemura
00:08:21.25 +02:56:19.6 14.7mag 78P/Gehrels
21:36:49.99 -16:53:09.1 14.5mag 88P/Howell
00:59:22.08 +13:03:44.9 15.2mag 93P/Lovas
04:09:46.78 +30:38:55.2 16.5mag 123P/West-Hartley
08:07:39.26 +50:30:37.7 16.2mag 124P/Mrkos
01:53:32.68 +11:17:19.1 16.4mag 128P/Shoemaker-Holt
01:56:21.48 +10:57:16.0 17.4mag 131P/Mueller
23:17:40.53 +02:52:41.2 13.0mag 141P/Machholz
23:27:45.54 -04:36:28.4 13.1mag 141P-A/Machholz
22:28:52.11 -07:06:47.7 16.2mag 141P-D/Machholz
23:48:52.45 -14:24:07.0 15.5mag 162P/SidingSpring
10:39:44.55 +32:02:10.3 17.5mag 164P/Christensen
05:48:47.49 +24:44:24.5 17.5mag 198P/ODAS
15:34:02.53 -03:26:58.5 16.9mag 210P/Christensen
20:09:42.13 -17:39:51.8 17.1mag 218P/LINEAR
16:58:40.59 -16:43:22.2 16.3mag 235P/LINEAR
04:40:24.21 +31:55:36.9 16.3mag 240P/NEAT
07:29:48.12 -08:26:55.4 17.5mag 242P/Spahr
15:48:35.97 +05:03:46.9 17.7mag 391P/Kowalski
07:27:57.13 +21:05:52.5 17.5mag 450P/LONEOS
05:00:18.01 +46:39:13.2 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 20 05:48 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
-rw-r--r-- 1 apache apache 5.7K Mar 20 05:48 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
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
-rw-r--r-- 1 apache apache 187K Mar 20 05:48 tocp_transients_list.txt
