This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm
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
NSV 25427,2461126.8687,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 25427 20260327.3687 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:06.69 +50:08:00.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_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
V2266 Cyg,2461126.8687,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2266 Cyg 20260327.3687 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:24.83 +55:22:11.2 ;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-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_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 J212803.73+521335.8,2461126.8687,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212803.73+521335.8 20260327.3687 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:03.64 +52:13:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2138529+532943,2461126.8687,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2138529+532943 20260327.3687 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:53.26 +53:29:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_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
V1548 Cyg,2461126.8687,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1548 Cyg 20260327.3687 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:54.90 +51:34:38.2 ;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-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2126544+572224,2461126.8687,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2126544+572224 20260327.3687 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:54.42 +57:22:26.1 ;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-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_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
V1047 Cep,2461126.8687,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1047 Cep 20260327.3687 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:09.63 +55:35:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20_00sec_-15_00C_LIGHT_0374_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20_00sec_-15_00C_LIGHT_0373_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: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461126.86894681 27.03.2026 08:51:07.004 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
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: 5 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): 21807
Objects passed selection criteria: 21672
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 14630.2
Average stars matched: 13787 (94.2363 %)
Memory usage VmPeak: 126060 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 03:54:32 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: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461126.86894681 27.03.2026 08:51:07.004 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
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: 26 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): 148545
Objects passed selection criteria: 148141
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 99776.8
Average stars matched: 93356.2 (93.5651 %)
Memory usage VmPeak: 2042600 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 03:57:26 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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: 2461126.86839248
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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:33.744 +54:00:30.08
Angular distance between the image centers 0.01 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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:34.407 +53:59:57.90
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:10:33.744 +54:00:30.08
Second-epoch second image center 21:10:34.407 +53:59:57.90
Angular distance between the image centers 0.00908 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.V74piR5YRk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.D1rtvUFfax
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits &> /tmp/tmp.qF11uF2pxv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits &> /tmp/tmp.s57Gb7kV8e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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 13689 out of 25856 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.933084
a=0.000000 b=1.000000 c=22.933084
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.93
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.4 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
3.6 pix fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
3.5 pix fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Limiting magnitude estimates:
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
13.5 mag. fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
13.6 mag. fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 11.0 (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.V74piR5YRk (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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3218, passed=25856
Got 25856 stars (including 22610 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 25856 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 972 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: 0.52"
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 972 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: 0.50"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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.D1rtvUFfax (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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3203, passed=25854
Got 25854 stars (including 22628 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 25854 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 974 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: 0.54"
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 974 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: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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.qF11uF2pxv (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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=369, passed=9048
Got 9048 stars (including 8670 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat
util/solve_plate_with_UCAC5 got 9048 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 954 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_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.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.s57Gb7kV8e (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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, passed=8790
Got 8790 stars (including 8420 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat
util/solve_plate_with_UCAC5 got 8790 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.77"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 955 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits'
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out23987.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23987_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
Preparing report for the candidate 23987_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Cyg-02-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 ####
21:01:06.69 +50:08:00.0
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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:33.744 +54:00:30.08
Angular distance between the image centers 0.01 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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:34.407 +53:59:57.90
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:10:33.744 +54:00:30.08
Second-epoch second image center 21:10:34.407 +53:59:57.90
Angular distance between the image centers 0.00908 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.CvFOIrsD5H
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.C0WsxrpDqQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits &> /tmp/tmp.UrrjrbBGU9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits &> /tmp/tmp.FuIW4ESA7Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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 14463 out of 180620 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.756732
a=0.000000 b=1.000000 c=22.756732
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
3.7 pix fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
3.4 pix fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Limiting magnitude estimates:
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
13.6 mag. fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
13.6 mag. fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.0 (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.CvFOIrsD5H (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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=28755, passed=180569
Got 180569 stars (including 151468 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 180569 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 973 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: 0.50"
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 973 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: 0.49"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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.C0WsxrpDqQ (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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=29011, passed=181061
Got 181061 stars (including 151708 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 181061 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 975 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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.UrrjrbBGU9 (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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3524, passed=50251
Got 50251 stars (including 46675 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat
util/solve_plate_with_UCAC5 got 50251 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 966 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: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 961 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.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.FuIW4ESA7Z (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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=3530, passed=51611
Got 51611 stars (including 48024 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat
util/solve_plate_with_UCAC5 got 51611 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 968 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: 0.74"
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 966 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: 0.80"
Excluding outliers - 963 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-50-19_20.00sec_-15.00C_LIGHT_0373.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.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-02-Q2b1x1_035205_TTUQ2b1x1_17175_EstHFWwm/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374.fits
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out205805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out106674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78940.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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
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Considering the candidate 205805_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 205805_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:37:20.41 +50:54:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.072 2171460255698958592 324.33413958415 +50.90646946084 12.6499 12.0383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205812_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 205812_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:20:14.98 +56:44:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.163 2178898658016200832 320.06195253957 +56.73809964794 12.4013 11.2048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205813_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 205813_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:31:35.28 +57:31:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.047 2178809253979714944 322.89608162208 +57.52314416279 12.8957 12.2665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205819_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 205819_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:38:07.55 +54:55:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205820_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 205820_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 208316_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 208316_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:01:48.72 +57:05:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.303 2189665419472802432 315.45358485246 +57.09988854154 11.7532 11.1622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208882_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 208882_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:03:43.86 +53:15:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209237_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 209237_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:39:12.10 +57:29:56.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 209684_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 209684_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:27:54.41 +53:19:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209737_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 209737_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:29:02.90 +51:14:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209836_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 209836_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:38:51.01 +57:27:33.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 210231_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 210231_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:39:45.57 +55:22:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210819_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 210819_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:32:59.76 +49:57:23.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 211224_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211224_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:13:50.14 +52:43:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211331_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211331_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:02:21.74 +56:39:57.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 211553_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211553_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:01:54.75 +57:06:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211564_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211564_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:11:30.16 +53:44:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211627_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211627_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:50:06.94 +56:48:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211654_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211654_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:17:49.82 +52:29:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 4.242 2175406265483846272 319.45785048299 +52.49627828491 12.5112 11.6339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211683_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211683_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:52:22.44 +55:01:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.537 2174052491799239424 328.09303755627 +55.02480419966 12.3572 11.8917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211887_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211887_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:24:50.36 +50:15:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211908_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 211908_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:01:39.88 +57:45:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212340_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 212340_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:30:27.62 +52:56:36.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212480_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 212480_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:11:19.09 +57:38:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.642 2189576359033590016 317.82832333396 +57.63394749920 12.8162 12.3465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212742_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 212742_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:44:12.58 +55:24:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213527_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 213527_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:10:04.91 +53:33:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213597_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 213597_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:29:02.07 +55:26:10.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213778_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 213778_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:20:13.75 +56:31:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213881_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 213881_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:32:29.21 +54:57:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214204_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 214204_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:58:24.29 +55:39:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214745_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 214745_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:59:40.05 +55:32:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.139 2188876588597280128 314.91705997136 +55.53608492591 13.2476 12.4402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215069_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 215069_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:11:20.39 +54:26:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135032_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 135032_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:34:23.95 +50:03:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74759_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 74759_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:32:45.05 +54:17:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43258_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
Preparing report for the candidate 43258_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
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Considering the candidate 103722_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 103722_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:23:29.89 +52:31:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79640_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 79640_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:05:22.66 +54:03:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24584_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 24584_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:42:03.67 +56:54:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106674_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
Preparing report for the candidate 106674_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
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Considering the candidate 134613_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 134613_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:13:05.74 +50:25:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57750_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 57750_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:35:55.39 +54:49:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23867_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 23867_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:24:40.29 +57:18:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78940_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
Preparing report for the candidate 78940_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
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Considering the candidate 174556_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 174556_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:01:06.67 +50:07:59.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 94836_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 94836_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:44:45.05 +53:16:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67289_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 67289_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:47:52.60 +53:54:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125047_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
Preparing report for the candidate 125047_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22744_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
Preparing report for the candidate 22744_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46334_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
Preparing report for the candidate 46334_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
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Considering the candidate 89843_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 89843_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:10:15.77 +53:33:48.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134116_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 134116_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:58:30.19 +50:27:45.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 24538_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 24538_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 20:45:21.43 +57:34:39.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 179367_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 179367_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:32:56.60 +49:58:40.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15988_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 15988_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:38:57.62 +57:29:21.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23695_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 23695_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:54:53.12 +56:36:39.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 37004_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 37004_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks
**** FOUND 21:52:01.02 +55:47:43.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177065_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374
The candidate 177065_fd_Cyg-02-Q2b1x1_2026-03-27_03-51-07_20.00sec_-15.00C_LIGHT_0374 did not pass the final checks