This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W
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
VARIABLE_NAME,2461119.6767,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:04.56 +19:34:19.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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!
TCP 2026 03 20.1767* 09 44 38.00 +17 05 52.6 13.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6767,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:44:38.00 +17:05:52.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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
VARIABLE_NAME,2461119.6767,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:02:50.87 +22:29:13.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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!
TCP 2026 03 20.1767* 09 23 28.68 +19 55 56.9 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6767,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:23:28.68 +19:55:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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
VARIABLE_NAME,2461119.6767,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:02:19.09 +22:15:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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
VARIABLE_NAME,2461119.6767,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:43:03.16 +19:56:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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
VARIABLE_NAME,2461119.6767,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:44.59 +22:58:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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!
TCP 2026 03 20.1767* 09 23 53.99 +25 32 02.8 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6767,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:23:53.99 +25:32:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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!
TCP 2026 03 20.1767* 09 47 36.07 +26 29 49.2 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6767,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1767 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:47:36.07 +26:29:49.2 ;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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_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: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
First image: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Last image: 2461119.67704186 20.03.2026 04:14:46.417 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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: 4 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): 9353
Objects passed selection criteria: 9345
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 8957
Average stars matched: 8536.75 (95.3081 %)
Memory usage VmPeak: 114840 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 23:21:19 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: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
First image: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Last image: 2461119.67704186 20.03.2026 04:14:46.417 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 143
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 17 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): 49412
Objects passed selection criteria: 49294
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 47805.8
Average stars matched: 45593.5 (95.3724 %)
Memory usage VmPeak: 148444 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 23:22:14 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/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461119.67641736
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits exists and is non-empty
Saving wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits to local_wcs_cache/
'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits exists and is non-empty
Saving wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits to local_wcs_cache/
'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:14:05.815 +22:02:06.51
Angular distance between the image centers 0.07 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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:14:09.129 +22:02:28.14
Angular distance between the image centers 0.09 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 09:14:05.815 +22:02:06.51
Second-epoch second image center 09:14:09.129 +22:02:28.14
Angular distance between the image centers 0.01414 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/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits &> /tmp/tmp.iM8jspkVx8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits &> /tmp/tmp.dYLABxK1AQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.weIqzDCxbY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.nV5qUXvqPT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Found non-empty wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
The reference image (wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits) and catalog (wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat) found
'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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 4769 out of 8632 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.930105
a=0.000000 b=1.000000 c=22.930105
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
2.1 pix Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
2.5 pix fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
2.3 pix fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Limiting magnitude estimates:
15.3 mag. Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
15.3 mag. Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
15.3 mag. fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
15.4 mag. fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.iM8jspkVx8 (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/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=673, passed=8632
Got 8632 stars (including 7938 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
util/solve_plate_with_UCAC5 got 8632 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 955 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits -region wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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.dYLABxK1AQ (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/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=654, passed=8532
Got 8532 stars (including 7867 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
util/solve_plate_with_UCAC5 got 8532 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 956 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits -region wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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.weIqzDCxbY (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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=629, passed=9666
Got 9666 stars (including 9030 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 9666 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 956 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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.nV5qUXvqPT (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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=690, passed=9320
Got 9320 stars (including 8620 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 9320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 957 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_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20493.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20463_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 20463_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:19:04.95 +18:19:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 1.089 632561859937593984 139.77079613601 +18.32672751778 10.9650 10.5471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20482_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 20482_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:19:28.91 +25:10:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.519 687642272888501504 139.87040190261 +25.16894846649 12.3732 11.9184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20484_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 20484_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:17:33.15 +26:26:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.802 694709555675281280 139.38868385422 +26.44501275927 12.5471 12.0564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20489_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 20489_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:12:25.41 +22:01:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20490_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 20490_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:50:32.04 +20:50:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.569 661705923164653568 132.63348693895 +20.83835195853 12.2524 11.3968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20493_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 20493_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:52:37.41 +25:26:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.849 690137580168527616 133.15593106585 +25.44063064181 12.6117 12.1140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01624_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 01624_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:09:52.67 +25:14:52.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cnc-03-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 ####
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/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits exists and is non-empty
wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:14:05.815 +22:02:06.51
Angular distance between the image centers 0.07 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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:14:09.129 +22:02:28.14
Angular distance between the image centers 0.09 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 09:14:05.815 +22:02:06.51
Second-epoch second image center 09:14:09.129 +22:02:28.14
Angular distance between the image centers 0.01414 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/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits &> /tmp/tmp.z2mAHONqjn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits &> /tmp/tmp.ux3UPpIfOR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.ii8l9lj2Lx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.BJRrjr0OY5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Found non-empty wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
The reference image (wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits) and catalog (wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat) found
'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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 4825 out of 48025 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.818214
a=0.000000 b=1.000000 c=22.818214
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
2.0 pix Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
2.4 pix fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
2.2 pix fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Limiting magnitude estimates:
15.5 mag. Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
15.4 mag. Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
15.4 mag. fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
15.5 mag. fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.z2mAHONqjn (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/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
SExtractor catalog parsing summary: zero_flux=11, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2316, passed=47999
Got 47999 stars (including 45610 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
util/solve_plate_with_UCAC5 got 47999 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 955 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits -region wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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.ux3UPpIfOR (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/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=2292, passed=48027
Got 48027 stars (including 45647 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
util/solve_plate_with_UCAC5 got 48027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 957 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_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits -region wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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.ii8l9lj2Lx (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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=2696, passed=47327
Got 47327 stars (including 44579 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 47327 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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.BJRrjr0OY5 (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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=2712, passed=49370
Got 49370 stars (including 46582 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 49370 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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_2026-03-19_CI_Cnc-03-Q2b1x1_231542_TTUQ2b1x1_8266_MW3wD06W/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53739.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 53411_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53411_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:38:36.25 +21:13:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.206 640710409330515072 144.65063324478 +21.23050808706 14.5187 14.0125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53415_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53415_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:40:48.01 +24:49:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.537 644821998702521728 145.19998722734 +24.83266849847 14.2441 13.6920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53417_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53417_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:52:24.22 +19:18:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.772 660662765804533248 133.10070554835 +19.31027355845 14.4729 13.9774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53419_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53419_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:46:24.79 +19:43:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.405 661159916858658816 131.60365743560 +19.72481602157 14.3876 14.0178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53424_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53424_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:40:22.92 +26:59:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.806 703432565534494592 130.09609486955 +26.98398396727 13.7822 13.5322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53425_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53425_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:55:27.67 +18:31:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.716 660352188129120256 133.86518515594 +18.52924523369 14.1999 13.6297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53426_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53426_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:51:20.71 +17:21:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.911 611778581912146304 132.83655418635 +17.35799173310 14.3356 13.9287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53432_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53432_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:00:34.84 +17:55:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.092 612046347352935424 135.14544591663 +17.92187785567 13.4070 12.6558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53433_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53433_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:46:14.36 +24:37:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.098 643261241946863872 146.55981381610 +24.62339586588 13.4178 12.9109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53435_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53435_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:48:32.83 +25:57:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.049 691068282402286592 132.13711447211 +25.96483645772 13.2269 12.7723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53485_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53485_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:05:00.98 +22:48:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.210 685643429469312000 136.25407810102 +22.81080295431 12.7743 12.1540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53538_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53538_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53550_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53550_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53575_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53575_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:43:05.11 +19:27:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.975 661043918382057344 130.77072810799 +19.45819253245 13.4435 12.6433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53632_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53632_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53649_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53649_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53679_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53679_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:28:03.04 +25:56:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53680_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53680_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53688_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53688_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:43:30.17 +19:13:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.574 661025639001254272 130.87561238300 +19.22832227179 14.3919 13.7254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53720_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53720_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53721_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53721_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:54:31.88 +22:50:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.200 686204523996508928 133.63318790244 +22.84498960195 14.3383 13.8317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53727_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53727_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53733_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53733_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:46:34.51 +17:10:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.232 658344067579600128 131.64408259901 +17.17361259722 14.3174 13.8776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53737_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53737_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53739_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53739_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53770_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53770_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:43:20.43 +20:37:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 4.717 661461595361847424 130.83613005665 +20.62905097558 14.7502 14.2675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53777_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53777_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 08:54:02.21 +23:31:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.185 689619847630787584 133.50979752384 +23.51680679607 14.6983 14.2283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53794_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 53794_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 09:37:48.50 +20:25:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.350 634597090320338048 144.45172356037 +20.42535836272 14.1436 13.6052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08312_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145
The candidate 08312_fd_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks