This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv
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!
TCP 2026 03 26.3040* 16 20 22.94 -01 40 10.7 13.0 U Ser 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,2461125.8040,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3040 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:20:22.94 -01:40:10.7 ;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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_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 26.3040* 16 08 29.50 -03 09 17.4 13.2 U Ser 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,2461125.8040,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3040 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:08:29.50 -03:09:17.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164046.96-032822.1,2461125.8040,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J164046.96-032822.1 20260326.3040 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:40:46.98 -03:28:21.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_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 26.3040* 16 15 00.05 -01 19 13.2 13.9 U Ser 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,2461125.8040,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3040 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:00.05 -01:19:13.2 ;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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_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,2461125.8040,14.58,0.05,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 20260326.3040 14.58CV 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:29:56.59 -02:35:26.7 ;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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20_00sec_-10_00C_LIGHT_0563_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20_00sec_-10_00C_LIGHT_0562_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: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
First image: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Last image: 2461125.80433521 26.03.2026 07:18:04.562 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
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: 6 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): 7096
Objects passed selection criteria: 7088
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 6161.5
Average stars matched: 5988.25 (97.1882 %)
Memory usage VmPeak: 113572 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 02:23:08 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: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
First image: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Last image: 2461125.80433521 26.03.2026 07:18:04.562 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 75
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 21 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): 48074
Objects passed selection criteria: 47985
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 43664
Average stars matched: 42058.2 (96.3225 %)
Memory usage VmPeak: 150688 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 02:24:01 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat to cache
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.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: 2461125.80374234
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits exists and is non-empty
Saving wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits to local_wcs_cache/
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> 'local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits exists and is non-empty
Saving wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits to local_wcs_cache/
'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> 'local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits exists and is non-empty
Saving wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits to local_wcs_cache/
'wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits' -> 'local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits'
wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits exists and is non-empty
Saving wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits to local_wcs_cache/
'wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits' -> 'local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:10.117 -02:00:18.98
Angular distance between the image centers 0.00 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 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:13.477 -01:59:45.82
Angular distance between the image centers 0.02 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 16:17:10.117 -02:00:18.98
Second-epoch second image center 16:17:13.477 -01:59:45.82
Angular distance between the image centers 0.01675 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits &> /tmp/tmp.gbMTLhWO1a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits &> /tmp/tmp.MwKPHbwCSa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits &> /tmp/tmp.89Cj35NzZm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits &> /tmp/tmp.D6MLSnSD52
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
The reference image (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits) and catalog (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat) found
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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 4442 out of 8868 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.923574
a=0.000000 b=1.000000 c=22.923574
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
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:
2.4 pix Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
2.4 pix Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
2.4 pix fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
2.4 pix fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Limiting magnitude estimates:
15.0 mag. Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
15.0 mag. Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
14.6 mag. fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
14.6 mag. fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gbMTLhWO1a (6) ############
Parsing command line arguments...
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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=511, passed=8867
Got 8867 stars (including 8350 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
util/solve_plate_with_UCAC5 got 8867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 970 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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.MwKPHbwCSa (6) ############
Parsing command line arguments...
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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=557, passed=8941
Got 8941 stars (including 8375 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
util/solve_plate_with_UCAC5 got 8941 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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.89Cj35NzZm (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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=383, passed=6020
Got 6020 stars (including 5627 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat
util/solve_plate_with_UCAC5 got 6020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 966 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 - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.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.D6MLSnSD52 (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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=365, passed=6091
Got 6091 stars (including 5717 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat
util/solve_plate_with_UCAC5 got 6091 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 966 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 - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
Saving fully-calibrated image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits'
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits'
Preparing the HTML report for the field Ser-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 20508_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 20508_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:07:08.15 -00:18:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20559_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 20559_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:30:56.18 +01:57:04.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20595_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 20595_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:34:46.89 -01:30:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01667_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 01667_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:30:49.46 -05:30:19.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ser-06-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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat to cache
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Creating symlink local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits exists and is non-empty
wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits exists and is non-empty
wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits exists and is non-empty
wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:10.117 -02:00:18.98
Angular distance between the image centers 0.00 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 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:13.477 -01:59:45.82
Angular distance between the image centers 0.02 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 16:17:10.117 -02:00:18.98
Second-epoch second image center 16:17:13.477 -01:59:45.82
Angular distance between the image centers 0.01675 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits &> /tmp/tmp.GJ2c8oG46m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits &> /tmp/tmp.K3NcWXJHyf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits &> /tmp/tmp.28PXfITEFm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits &> /tmp/tmp.BupNfkRwqP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
The reference image (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits) and catalog (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat) found
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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 4513 out of 57255 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.756312
a=0.000000 b=1.000000 c=22.756312
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
2.2 pix Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
2.2 pix fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
2.2 pix fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Limiting magnitude estimates:
15.2 mag. Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
15.2 mag. Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
14.8 mag. fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
14.7 mag. fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GJ2c8oG46m (6) ############
Parsing command line arguments...
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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=3363, passed=57246
Got 57246 stars (including 53818 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
util/solve_plate_with_UCAC5 got 57246 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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.K3NcWXJHyf (6) ############
Parsing command line arguments...
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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3390, passed=57768
Got 57768 stars (including 54311 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
util/solve_plate_with_UCAC5 got 57768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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.28PXfITEFm (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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1786, passed=42627
Got 42627 stars (including 40787 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat
util/solve_plate_with_UCAC5 got 42627 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 967 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: 0.44"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.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.BupNfkRwqP (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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1882, passed=41943
Got 41943 stars (including 40025 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat
util/solve_plate_with_UCAC5 got 41943 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 965 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: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Saving fully-calibrated image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-17-13_20.00sec_-10.00C_LIGHT_0562.fits
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.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_2026-03-26_CI_Ser-06-Q2b1x1_022050_TTUQ2b1x1_8754_ZAIv6JUv/wcs_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563.fits
Preparing the HTML report for the field Ser-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out67383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out72370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73280.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 3s
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Considering the candidate 71858_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71858_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:28:38.80 -00:27:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.454 4359442559070854272 247.16179245959 -00.46302082298 14.0620 13.4450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71861_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71861_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:31:30.96 -00:01:19.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)
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Considering the candidate 71862_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71862_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 15:50:16.20 -00:18:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.721 4410275799120141952 237.56752000317 -00.30138407783 14.0298 13.4694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71864_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71864_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:32:40.71 -04:40:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 3.138 4354243965016199680 248.17034413105 -04.67177379256 13.9888 13.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71866_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71866_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:40:32.86 -01:16:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.866 4382328412566980736 250.13642859238 -01.27396423385 13.6213 13.0688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71868_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71868_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:39:06.09 +01:04:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.511 4384025852362300160 249.77550872450 +01.08234116155 13.9439 13.3721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71871_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71871_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:40:09.65 -02:50:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.309 4354940333833627520 250.04073480087 -02.83785306310 13.8478 13.1859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71878_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71878_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:40:00.72 +00:09:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.887 4383334362627081728 250.00249897769 +00.16112592061 14.0671 13.4304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71880_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71880_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:41:16.02 +00:58:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.223 4383824126338191872 250.31643121993 +00.97049362560 13.4376 12.7512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71881_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71881_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:41:29.91 -00:33:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.482 4382483856023141248 250.37425438977 -00.55492914372 13.6236 12.8446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71883_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71883_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:37:32.15 +00:42:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 71884_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71884_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:14:54.84 -01:02:02.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 71885_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71885_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:06:28.59 +01:37:49.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 71887_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71887_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:41:39.05 +00:22:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.577 4383708162221289984 250.41310449283 +00.38090916221 13.3114 12.5649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71889_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71889_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:41:03.97 +01:57:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.604 4384224417290581504 250.26609984685 +01.95585672119 13.4018 12.8264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71891_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71891_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 71892_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71892_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:29:09.06 -00:58:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.863 4359362500880338944 247.28754630005 -00.98004292270 13.0358 12.4869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71894_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 71894_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 15:55:30.75 -05:50:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 0.272 4398099223242395264 238.87815257189 -05.84509612793 12.6796 12.0646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72251_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 72251_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:02:58.22 -05:49:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.461 4350297817787246976 240.74246316914 -05.82354610196 12.5650 11.9662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72370_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
Preparing report for the candidate 72370_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
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Considering the candidate 72397_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 72397_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:37:44.36 +01:27:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.262 4384097767294781952 249.43459219210 +01.45419001222 13.1054 12.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72442_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
Preparing report for the candidate 72442_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
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Considering the candidate 72570_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 72570_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:34:43.18 +00:59:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.252 4383681877021162752 248.67957251922 +00.98586655439 13.6367 13.0750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72642_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 72642_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:38:43.36 -01:11:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.811 4382342362620888192 249.68144555772 -01.19650210989 13.5081 12.8844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72685_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 72685_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:24:43.84 -02:29:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.747 4358494745688677760 246.18299186460 -02.49605946719 13.9530 13.3809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72719_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 72719_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:20:56.90 -00:24:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.734 4407634497313906560 245.23689954542 -00.40916202357 13.7645 13.1312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72809_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 72809_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:09:46.02 +00:47:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.793 4411434718738279552 242.44249352655 +00.79372889962 13.7796 13.2289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72820_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
Preparing report for the candidate 72820_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
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Considering the candidate 72951_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
Preparing report for the candidate 72951_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
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Considering the candidate 73280_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
Preparing report for the candidate 73280_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
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Considering the candidate 09179_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 09179_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:30:49.46 -05:30:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31057_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 31057_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:34:46.89 -01:30:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67383_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 67383_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:40:28.90 +01:20:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.649 4384037255498163328 250.12023870379 +01.34311177610 12.9652 12.2606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 30764_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 30764_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks
**** FOUND 16:19:37.30 -01:15:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37930_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563
The candidate 37930_fd_Ser-06-Q2b1x1_2026-03-26_02-18-04_20.00sec_-10.00C_LIGHT_0563 did not pass the final checks