This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG
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
DM Cyg,2461126.9128,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DM Cyg 20260327.4128 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:11.57 +32:11:28.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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
V0597 Vul,2461126.9128,9.87,0.05,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
V0597 Vul 20260327.4128 9.87CV 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:58.05 +27:23:55.9 ;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-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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 1856108982132748160,2461126.9128,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1856108982132748160 20260327.4128 13.24CV 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:17.33 +26:41:35.5 ;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-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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 1864897619098702976,2461126.9128,13.12,0.05,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 1864897619098702976 20260327.4128 13.12CV 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:57:01.64 +31:42:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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 1853460980173329152,2461126.9128,12.88,0.05,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 1853460980173329152 20260327.4128 12.88CV 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:21.70 +31:19:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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 1860980643283648896,2461126.9128,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1860980643283648896 20260327.4128 12.96CV 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:32:37.59 +30:11:44.0 ;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-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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 1869012575726671488,2461126.9128,12.88,0.05,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 1869012575726671488 20260327.4128 12.88CV 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:47:54.55 +33:02:46.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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,2461126.9128,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4128 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:48:09.28 +26:16:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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
UW Vul,2461126.9128,10.82,0.05,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
UW Vul 20260327.4128 10.82CV 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:52:32.01 +27:10:30.2 ;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-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212217.27+293729.0,2461126.9128,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212217.27+293729.0 20260327.4128 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:17.11 +29:37:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_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
ASAS J210219+2752.7,2461126.9128,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J210219+2752.7 20260327.4128 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:19.39 +27:52:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20_00sec_-15_00C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.54827539 27.12.2025 01:09:20.994 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
First image: 2461036.54827539 27.12.2025 01:09:20.994 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Last image: 2461126.91308984 27.03.2026 09:54:40.962 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.04
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): 21785
Objects passed selection criteria: 21712
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: 16977.2
Average stars matched: 15914.8 (93.7416 %)
Memory usage VmPeak: 125432 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 05:36:12 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.54827539 27.12.2025 01:09:20.994 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
First image: 2461036.54827539 27.12.2025 01:09:20.994 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Last image: 2461126.91308984 27.03.2026 09:54:40.962 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 130
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
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: 61 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): 162226
Objects passed selection criteria: 161810
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 121580
Average stars matched: 114525 (94.1972 %)
Memory usage VmPeak: 1987220 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 05:40:23 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
SExtractor catalog cache: saved Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.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: 2461126.91255650
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits exists and is non-empty
Saving wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits'
wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits exists and is non-empty
Saving wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits'
wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits exists and is non-empty
Saving wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits to local_wcs_cache/
'wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits' -> 'local_wcs_cache/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits'
wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits exists and is non-empty
Saving wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits to local_wcs_cache/
'wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits' -> 'local_wcs_cache/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:00:00.467 +30:00:01.62
Second-epoch image center 20:59:53.666 +29:57:55.24
Angular distance between the image centers 0.04 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 21:00:00.467 +30:00:01.62
Second-epoch image center 20:59:53.833 +29:58:12.58
Angular distance between the image centers 0.04 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 20:59:53.666 +29:57:55.24
Second-epoch second image center 20:59:53.833 +29:58:12.58
Angular distance between the image centers 0.00485 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits &> /tmp/tmp.Ymr2juyCp7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits &> /tmp/tmp.wBPSQYjnUy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits &> /tmp/tmp.8l5wBBBa2S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits &> /tmp/tmp.cahpy0NmGs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits and wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits and wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
Found non-empty wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits and wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
The reference image (wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits) and catalog (wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat) found
'wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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 17081 out of 25079 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.936691
a=0.000000 b=1.000000 c=22.936691
From vast_summary.log: estimated ref. image limiting mag.: -8.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
2.4 pix Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
3.5 pix fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
3.4 pix fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Limiting magnitude estimates:
14.9 mag. Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
14.9 mag. Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
14.0 mag. fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
14.1 mag. fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Ymr2juyCp7 (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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits' -> 'wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Checking if the catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WCS catalog name: wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2527, passed=25079
Got 25079 stars (including 22522 good ones) from the SExtractor catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 25079 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits -region wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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.wBPSQYjnUy (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-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits' -> 'wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
Checking if the catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WCS catalog name: wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2509, passed=25067
Got 25067 stars (including 22525 good ones) from the SExtractor catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 25067 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits -region wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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.8l5wBBBa2S (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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS-calibrated image found: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
Checking if the catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS catalog name: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=620, passed=14296
Got 14296 stars (including 13669 good ones) from the SExtractor catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
util/solve_plate_with_UCAC5 got 14296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits -region wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.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.cahpy0NmGs (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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
WCS-calibrated image found: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Checking if the catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
WCS catalog name: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=671, passed=14620
Got 14620 stars (including 13944 good ones) from the SExtractor catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat
util/solve_plate_with_UCAC5 got 14620 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 939 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits -region wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits'
Saving fully-calibrated image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits'
Saving fully-calibrated image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits'
Preparing the HTML report for the field Cyg-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out07883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19122.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32214_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 32214_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:05:59.70 +29:24:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32262_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 32262_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:42:22.13 +27:28:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32368_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 32368_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:09:23.82 +26:40:17.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32601_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 32601_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:08:05.95 +32:13:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33572_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 33572_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:13:51.81 +28:47:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07883_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 07883_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17475_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 17475_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:46:18.84 +28:15:44.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19122_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 19122_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09278_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 09278_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:49:01.25 +31:50:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16018_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 16018_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:18:18.22 +28:40:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12456_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 12456_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:12:56.05 +30:13:34.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19749_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 19749_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:52:07.74 +27:05:50.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cyg-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:21:11.57 +32:11:28.5
21:04:58.05 +27:23:55.9
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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
SExtractor catalog cache: saved Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits exists and is non-empty
wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits exists and is non-empty
wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:00:00.467 +30:00:01.62
Second-epoch image center 20:59:53.666 +29:57:55.24
Angular distance between the image centers 0.04 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 21:00:00.467 +30:00:01.62
Second-epoch image center 20:59:53.833 +29:58:12.58
Angular distance between the image centers 0.04 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 20:59:53.666 +29:57:55.24
Second-epoch second image center 20:59:53.833 +29:58:12.58
Angular distance between the image centers 0.00485 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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits &> /tmp/tmp.XXn2OyJQZx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits &> /tmp/tmp.Ik0RQSg0jk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits &> /tmp/tmp.5AJqy9efIo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits &> /tmp/tmp.D7V5ZMAG5a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits and wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits and wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
Found non-empty wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits and wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
The reference image (wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits) and catalog (wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat) found
'wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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 18914 out of 194611 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.752848
a=0.000000 b=1.000000 c=22.752848
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.06
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 96 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
2.2 pix Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
3.6 pix fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
3.5 pix fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Limiting magnitude estimates:
15.1 mag. Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
15.0 mag. Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
14.0 mag. fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
14.1 mag. fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XXn2OyJQZx (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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits' -> 'wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Checking if the catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
WCS catalog name: wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=70, blended=28601, passed=194541
Got 194541 stars (including 165665 good ones) from the SExtractor catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 194541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits -region wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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.Ik0RQSg0jk (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-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits' -> 'wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
Checking if the catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
WCS catalog name: wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=28438, passed=192051
Got 192051 stars (including 163318 good ones) from the SExtractor catalog wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 192051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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: 0.49"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 953 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_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits -region wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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.5AJqy9efIo (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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS-calibrated image found: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
Checking if the catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS catalog name: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=7765, passed=80161
Got 80161 stars (including 72344 good ones) from the SExtractor catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
util/solve_plate_with_UCAC5 got 80161 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 926 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits -region wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.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.D7V5ZMAG5a (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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
WCS-calibrated image found: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Checking if the catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
WCS catalog name: wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=8164, passed=83898
Got 83898 stars (including 75668 good ones) from the SExtractor catalog wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat
util/solve_plate_with_UCAC5 got 83898 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 931 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits -region wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.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-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits
Saving fully-calibrated image wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_Cyg-09-Q2b1x1_2025-12-26_19-10-09_20.00sec_-15.00C_LIGHT_0011.fits
Saving fully-calibrated image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-53-54_20.00sec_-14.90C_LIGHT_0446.fits
Saving fully-calibrated image wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.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_2026-03-27_CI_Cyg-09-Q2b1x1_052941_TTUQ2b1x1_8224_FTetaJpG/wcs_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447.fits
Preparing the HTML report for the field Cyg-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out219651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out224624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out227033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out105525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219677.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 5s
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Considering the candidate 219651_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219651_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:40:38.62 +31:01:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.642 1862392897248856832 310.16024290385 +31.02428044393 13.4964 12.7994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219654_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 219654_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 219656_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219656_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:23:37.64 +31:26:00.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 219664_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 219664_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 219665_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219665_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:22:27.07 +30:26:48.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 219666_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 219666_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 219667_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219667_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:39:56.67 +33:23:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.158 1863221271874788096 309.98683738731 +33.39423087109 12.8126 12.3754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219672_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 219672_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 219673_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219673_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 219675_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219675_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:36:57.76 +31:13:57.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)
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Considering the candidate 219677_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 219677_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 219683_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219683_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:00:14.26 +28:52:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 5.234 1846342295220792192 315.06018037924 +28.86990214758 12.7287 12.1948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219685_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 219685_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 221990_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 221990_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:13:18.03 +32:03:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223521_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 223521_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 223611_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 223611_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:11:56.83 +30:39:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224095_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 224095_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:57:13.30 +33:12:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224624_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 224624_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:03:27.83 +27:19:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.821 1845128159505690496 315.86651191390 +27.32656243372 12.0483 11.2915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225605_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 225605_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 226176_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 226176_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:08:09.49 +32:08:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226324_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 226324_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:52:02.37 +27:04:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226538_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 226538_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 226800_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 226800_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 226844_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 226844_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:13:31.81 +32:45:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226862_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 226862_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 226909_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 226909_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 227033_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 227033_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:08:01.55 +32:38:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 5.171 1865226441790288000 317.00601000946 +32.64155841728 13.2196 12.6662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 227096_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 227096_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:51:58.94 +27:04:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227524_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 227524_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:21:18.83 +32:37:56.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 227565_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 227565_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:53:28.92 +31:31:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227602_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 227602_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:51:36.79 +28:13:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227716_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 227716_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 227997_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 227997_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:54:20.92 +28:03:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228119_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 228119_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:51:00.01 +33:04:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.703 1866021624916961280 312.75059408404 +33.06894499121 13.1034 12.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228251_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 228251_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 228540_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 228540_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:11:59.70 +30:38:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228556_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 228556_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:06:23.26 +31:11:58.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 228661_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 228661_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:22:22.35 +30:03:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228681_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 228681_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:20:22.56 +33:30:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229194_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 229194_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 229353_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 229353_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 229373_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 229373_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:57:09.06 +31:20:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229859_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 229859_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 229871_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 229871_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 229886_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 229886_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:41:50.60 +33:06:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229923_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 229923_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 230008_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 230008_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:45:33.15 +27:15:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230076_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 230076_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 230188_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 230188_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 230582_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 230582_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 230866_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 230866_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 230911_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 230911_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 230950_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 230950_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231001_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231001_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231149_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231149_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:54:19.28 +29:40:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231247_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231247_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231254_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231254_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231292_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231292_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231334_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231334_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231494_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231494_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231539_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231539_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231541_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231541_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231546_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231546_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 231562_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 231562_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 144617_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 144617_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:52:07.75 +27:05:50.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101313_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 101313_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:12:56.06 +30:13:34.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 91244_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 91244_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:58:44.63 +30:38:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116634_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 116634_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:48:19.97 +29:18:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78596_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 78596_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:17:09.38 +31:07:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136337_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 136337_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:46:18.84 +28:15:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69813_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 69813_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:49:01.13 +31:50:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194043_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 194043_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:04:58.04 +27:23:56.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 72222_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 72222_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:50:09.87 +31:40:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174447_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 174447_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 189479_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 189479_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 59722_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 59722_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:08:05.93 +32:13:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214999_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 214999_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 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 46509_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 46509_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:46:59.04 +33:00:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139702_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 139702_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:02:25.05 +28:01:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183281_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 183281_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:09:23.82 +26:40:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145959_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 145959_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:42:22.12 +27:28:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 206713_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 206713_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:04:05.45 +26:32:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123656_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 123656_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:13:51.81 +28:47:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105525_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 105525_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 114355_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 114355_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:05:59.70 +29:24:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124845_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 124845_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:18:18.21 +28:40:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73314_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 73314_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:10:14.76 +31:29:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142648_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
Preparing report for the candidate 142648_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
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Considering the candidate 57464_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 57464_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:21:11.56 +32:11:28.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 82866_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 82866_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:06:30.29 +31:11:04.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 100264_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 100264_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 21:08:38.97 +30:12:20.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 142753_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 142753_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:54:33.79 +28:03:29.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 93644_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 93644_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:45:40.10 +30:43:11.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 41657_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 41657_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:53:54.03 +33:26:15.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62125_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 62125_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks
**** FOUND 20:41:02.86 +32:18:25.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32929_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447
The candidate 32929_fd_Cyg-09-Q2b1x1_2026-03-27_04-54-40_20.00sec_-15.00C_LIGHT_0447 did not pass the final checks