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_032747_TTUQ2b1x1_10485_MipV0VYt
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
Gaia DR3 703248397336404608,2461118.8354,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 703248397336404608 20260319.3354 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:42:40.46 +26:51:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8354,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3354 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:41:04.89 +26:08:27.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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,2461118.8354,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:13.46 +19:34:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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 19.3354* 09 45 05.65 +17 05 00.7 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,2461118.8354,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:45:05.65 +17:05:00.7 ;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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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 19.3354* 09 23 50.48 +19 53 50.8 13.7 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,2461118.8354,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:23:50.48 +19:53:50.8 ;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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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,2461118.8354,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:03.95 +22:29:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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 19.3354* 09 24 08.38 +25 32 03.2 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,2461118.8354,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:24:08.38 +25:32:03.2 ;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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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 19.3354* 09 47 56.37 +26 25 41.5 13.9 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,2461118.8354,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:47:56.37 +26:25:41.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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,2461118.8354,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:02:36.99 +22:16:53.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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,2461118.8354,14.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 14.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:43:17.35 +19:56:27.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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,2461118.8354,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3354 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:54.51 +23:00:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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_03-03-11_20_00sec_-15_00C_LIGHT_0065_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_03-02-26_20_00sec_-14_90C_LIGHT_0064_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: 2461118.83566514 19.03.2026 08:03:11.468 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
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: 3 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): 8648
Objects passed selection criteria: 8646
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 8394.5
Average stars matched: 8200.75 (97.6919 %)
Memory usage VmPeak: 114344 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 03:30:36 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: 2461118.83566514 19.03.2026 08:03:11.468 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 310
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: 13 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): 45776
Objects passed selection criteria: 45684
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 42765.2
Average stars matched: 41715.2 (97.5447 %)
Memory usage VmPeak: 146692 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 03:31:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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: 2461118.83514018
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_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_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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 09:14:05.174 +22:00:35.38
Angular distance between the image centers 0.06 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 09:14:06.210 +22:00:49.60
Angular distance between the image centers 0.06 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 09:14:05.174 +22:00:35.38
Second-epoch second image center 09:14:06.210 +22:00:49.60
Angular distance between the image centers 0.00562 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.0b6xv7FOmj
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.saNqI0l3S9
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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits &> /tmp/tmp.nIPgxZfQtF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.PHWunhYxzI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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 4 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
2.6 pix fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
2.6 pix fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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
15.1 mag. fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
15.1 mag. fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (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.0b6xv7FOmj (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_032747_TTUQ2b1x1_10485_MipV0VYt/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.saNqI0l3S9 (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_032747_TTUQ2b1x1_10485_MipV0VYt/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.nIPgxZfQtF (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_032747_TTUQ2b1x1_10485_MipV0VYt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=450, passed=8364
Got 8364 stars (including 7906 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 8364 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 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: 0.44"
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 956 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: 0.42"
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_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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.PHWunhYxzI (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_032747_TTUQ2b1x1_10485_MipV0VYt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=437, passed=8348
Got 8348 stars (including 7904 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 8348 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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: 0.42"
Estimated accuracy of the plate solution: 0.40"
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_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/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_032747_TTUQ2b1x1_10485_MipV0VYt/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_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits'
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20477.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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20474_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 20474_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 09:12:25.41 +22:01:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.436 638757741103680640 138.10595715603 +22.02084422217 12.0495 11.3468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20476_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 20476_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 09:46:46.91 +23:21:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.568 641426358903463296 146.69528647933 +23.36613238238 12.1899 11.7020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20477_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 20477_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 09:24:31.83 +22:49:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.181 639012656002384128 141.13260896182 +22.82442406544 12.1981 11.6867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01624_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 01624_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 09:09:52.63 +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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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 09:14:05.174 +22:00:35.38
Angular distance between the image centers 0.06 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 09:14:06.210 +22:00:49.60
Angular distance between the image centers 0.06 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 09:14:05.174 +22:00:35.38
Second-epoch second image center 09:14:06.210 +22:00:49.60
Angular distance between the image centers 0.00562 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.lWnZs45oYE
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.xLWoJykEAD
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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits &> /tmp/tmp.9nFBrRZ2gj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.hP5hR6uQIN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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 177 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
2.5 pix fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
2.6 pix fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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
15.1 mag. fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
15.1 mag. fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.lWnZs45oYE (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_032747_TTUQ2b1x1_10485_MipV0VYt/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.xLWoJykEAD (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_032747_TTUQ2b1x1_10485_MipV0VYt/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.9nFBrRZ2gj (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_032747_TTUQ2b1x1_10485_MipV0VYt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1780, passed=38340
Got 38340 stars (including 36520 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 38340 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 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: 0.46"
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 955 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: 0.42"
Excluding outliers - 954 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_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.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.hP5hR6uQIN (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_032747_TTUQ2b1x1_10485_MipV0VYt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1784, passed=37906
Got 37906 stars (including 36083 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 37906 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 954 stars left (next iteration limit 1049)
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_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/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_032747_TTUQ2b1x1_10485_MipV0VYt/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_03-02-26_20.00sec_-14.90C_LIGHT_0064.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_032747_TTUQ2b1x1_10485_MipV0VYt/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.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_032747_TTUQ2b1x1_10485_MipV0VYt/wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53602.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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: 7s
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Considering the candidate 53370_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53370_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53371_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53371_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:43:29.85 +26:56:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.039 703243758771710208 130.87465770873 +26.93788731361 13.4495 12.8330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53374_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53374_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:43:53.04 +17:34:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 2.381 658567126705020544 130.97169372715 +17.58294206528 13.7675 13.2602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53378_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53378_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:44:30.86 +25:46:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.980 691093605529391104 131.12918914091 +25.77031950374 13.5606 13.1025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53379_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53379_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:41:09.67 +25:45:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.789 702743034305105280 130.29107023964 +25.75794864470 13.2996 12.8512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53386_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53386_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:43:34.99 +26:39:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.866 703183560510174080 130.89433455466 +26.66161249906 12.9810 12.4012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53387_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53387_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53391_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53391_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:41:33.50 +26:32:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.506 703202973762311808 130.39096472847 +26.53919025832 12.2703 11.5629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53392_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53392_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:44:40.52 +25:24:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.577 690662253373967360 131.16868697470 +25.41121506697 12.8447 12.3532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53405_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53405_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53407_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53407_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53409_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53409_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53410_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53410_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53415_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53415_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53416_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53416_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53421_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53421_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 53422_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53422_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 53423_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53423_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53424_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53424_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53425_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53425_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53426_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53426_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 53427_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53427_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53428_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53428_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53431_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53431_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53433_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53433_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53434_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53434_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 53435_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53435_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 53436_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53436_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 53438_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53438_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53439_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53439_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53440_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53440_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53442_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53442_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53444_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53444_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53445_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53445_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53446_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53446_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53447_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53447_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53448_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53448_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53451_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53451_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 53452_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53452_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 53454_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53454_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 53455_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53455_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53456_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53456_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53457_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53457_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53458_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53458_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53460_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53460_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53461_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53461_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53462_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53462_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53463_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53463_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53464_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53464_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53465_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53465_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53466_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53466_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53467_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53467_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53468_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53468_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53469_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53469_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53473_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53473_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53474_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53474_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53475_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53475_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 53476_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53476_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53477_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53477_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53478_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53478_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53481_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53481_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53482_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53482_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 53484_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53484_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53485_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53485_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53487_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53487_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 53488_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53488_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53489_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53489_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53491_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53491_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53492_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53492_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53494_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53494_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53495_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53495_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53496_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53496_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 53497_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53497_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53498_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53498_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53499_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53499_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53500_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53500_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53501_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53501_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53502_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53502_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 53503_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53503_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53504_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53504_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53506_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53506_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53507_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53507_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 53510_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53510_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53512_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53512_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53513_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53513_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53514_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53514_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53515_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53515_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53516_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53516_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53517_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53517_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53519_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53519_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53520_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53520_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53522_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53522_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 53523_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53523_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53524_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53524_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53527_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53527_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53528_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53528_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53530_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53530_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53532_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53532_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53533_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53533_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53534_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53534_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53535_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53535_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 53536_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53536_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 53537_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53537_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53538_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53538_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53539_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53539_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53542_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53542_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53543_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53543_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 08:52:29.92 +18:02:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53544_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53544_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53545_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53545_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53546_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53546_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53549_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53549_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 09:28:03.15 +25:56:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.205 693741985442124928 142.01271027655 +25.94370823720 13.9525 13.2958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53550_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53550_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53552_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53552_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53553_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53553_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 53554_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53554_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53556_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53556_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53558_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53558_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 53561_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53561_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53563_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53563_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 53564_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53564_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53566_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53566_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53567_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53567_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53568_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53568_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53569_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53569_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53570_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53570_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53571_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53571_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 53572_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53572_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 53573_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53573_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53575_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53575_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53576_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53576_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 53578_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53578_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53579_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53579_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53580_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53580_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53582_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53582_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53584_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53584_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53585_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53585_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53587_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53587_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 53588_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53588_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 53589_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53589_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53590_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53590_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53592_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53592_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53594_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53594_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53597_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53597_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 53599_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53599_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 53602_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
Preparing report for the candidate 53602_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
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Considering the candidate 53603_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53603_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53606_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53606_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 53607_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53607_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53608_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53608_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53609_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53609_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53612_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53612_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53613_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53613_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53614_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53614_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53615_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53615_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 53616_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53616_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53617_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53617_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 53619_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53619_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53621_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53621_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53623_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53623_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 53625_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53625_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53627_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53627_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 53628_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53628_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 53630_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53630_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53632_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53632_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 53633_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53633_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53635_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53635_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 53636_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53636_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 53643_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53643_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53646_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53646_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 53647_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53647_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53650_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53650_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53654_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53654_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 53661_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53661_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 53696_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53696_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53716_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 53716_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 08312_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 08312_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks
**** FOUND 09:09:52.63 +25:14:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07116_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065
The candidate 07116_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065 did not pass the final checks