This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.1531 2461126.6531 13.97 05:34:46.90 +51:36:46.9
159.50570 10.13647 galactic Aur Second-epoch detections are separated by 2.9" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J083.7011+51.6141 | 05:34:46.90 +51:36:46.9 (user input) | LPV (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
ATO J083.7011+51.6141,2461126.6531,13.97,0.05,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
ATO J083.7011+51.6141 20260327.1531 13.97CV 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:46.90 +51:36:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.6531,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.1531 14.59CV 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:44.98 +55:22:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.6531,14.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.1531 14.62CV 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:18.49 +54:33:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.6531,14.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.1531 14.79CV 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:03.58 +51:51:29.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_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
V0492 Aur,2461126.6531,13.54,0.05,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
V0492 Aur 20260327.1531 13.54CV 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:56.77 +52:02:32.2 ;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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20_00sec_-10_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20_00sec_-15_00C_LIGHT_0173_fits__*pix.png resample_wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20_00sec_-10_00C_LIGHT_0102_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: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
First image: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461126.65336125 27.03.2026 03:40:40.412 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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): 18348
Objects passed selection criteria: 18246
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 13544.8
Average stars matched: 12789 (94.4203 %)
Memory usage VmPeak: 122744 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 22:45:27 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: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
First image: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461126.65336125 27.03.2026 03:40:40.412 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 134
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 98 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): 135014
Objects passed selection criteria: 134638
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 102094
Average stars matched: 96000.2 (94.0317 %)
Memory usage VmPeak: 2747284 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 22:48:36 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
SExtractor catalog cache: saved Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.65285258
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
Saving wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits to local_wcs_cache/
'wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits exists and is non-empty
Saving wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits to local_wcs_cache/
'wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits exists and is non-empty
Saving wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits to local_wcs_cache/
'wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits' -> 'local_wcs_cache/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits'
wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits exists and is non-empty
Saving wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits to local_wcs_cache/
'wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits' -> 'local_wcs_cache/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:48.023 +54:00:28.99
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:48.203 +54:00:28.67
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:38:48.023 +54:00:28.99
Second-epoch second image center 05:38:48.203 +54:00:28.67
Angular distance between the image centers 0.00045 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00045 deg. (min. required shift: 0.00164 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.aaFuHLl0td
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits &> /tmp/tmp.hzPnU42hTC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits &> /tmp/tmp.3DgoDulJ8Q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits &> /tmp/tmp.VqkqiDTUuG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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 8307 out of 21171 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.946929
a=0.000000 b=1.000000 c=22.946929
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
2.0 pix Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
2.5 pix fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
2.5 pix fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Limiting magnitude estimates:
15.4 mag. Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
15.4 mag. Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
14.5 mag. fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
14.5 mag. fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
All-image limiting magnitude estimate: 14.5 (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.aaFuHLl0td (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1951, passed=21171
Got 21171 stars (including 19188 good ones) from the SExtractor catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 21171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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.hzPnU42hTC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> 'wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Checking if the catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS catalog name: wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1992, passed=21135
Got 21135 stars (including 19116 good ones) from the SExtractor catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 21135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 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: 0.38"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits -region wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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.3DgoDulJ8Q (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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=738, passed=10736
Got 10736 stars (including 9986 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 10736 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 940 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 939 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits -region wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.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.VqkqiDTUuG (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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Checking if the catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
WCS catalog name: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=740, passed=10778
Got 10778 stars (including 10028 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat
util/solve_plate_with_UCAC5 got 10778 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 940 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits -region wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
Saving fully-calibrated image wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
Saving fully-calibrated image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits'
Saving fully-calibrated image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits'
Preparing the HTML report for the field Aur-01-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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31147_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 31147_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Aur-01-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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
SExtractor catalog cache: saved Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Creating symlink local_wcs_cache/wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits exists and is non-empty
wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits exists and is non-empty
wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:48.023 +54:00:28.99
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:48.203 +54:00:28.67
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:38:48.023 +54:00:28.99
Second-epoch second image center 05:38:48.203 +54:00:28.67
Angular distance between the image centers 0.00045 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00045 deg. (min. required shift: 0.00164 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/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.scMPIwQU99
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits &> /tmp/tmp.EvYNnVIJyd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits &> /tmp/tmp.mzFmdqdfih
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits &> /tmp/tmp.baQDTjYcWe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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 8396 out of 155080 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.800893
a=0.000000 b=1.000000 c=22.800893
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 104 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
1.9 pix Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
2.3 pix fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
2.3 pix fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Limiting magnitude estimates:
15.6 mag. Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
15.6 mag. Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
14.7 mag. fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
14.7 mag. fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.scMPIwQU99 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=52, blended=17009, passed=155028
Got 155028 stars (including 137750 good ones) from the SExtractor catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 155028 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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.EvYNnVIJyd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> 'wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Checking if the catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS catalog name: wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=17172, passed=155805
Got 155805 stars (including 138361 good ones) from the SExtractor catalog wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 155805 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits -region wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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.mzFmdqdfih (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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=5012, passed=73367
Got 73367 stars (including 68251 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 73367 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 943 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits -region wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.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.baQDTjYcWe (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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Checking if the catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
WCS catalog name: wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=4921, passed=73180
Got 73180 stars (including 68167 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat
util/solve_plate_with_UCAC5 got 73180 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 945 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits -region wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_Aur-01-Q2b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Saving fully-calibrated image wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_Aur-01-Q2b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Saving fully-calibrated image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-39-56_20.00sec_-10.00C_LIGHT_0102.fits
Saving fully-calibrated image wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.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_Aur-01-Q2b1x1_224240_TTUQ2b1x1_9355_jEXI6MWD/wcs_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103.fits
Preparing the HTML report for the field Aur-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out178015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out181913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out187353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56837.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 4s
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Considering the candidate 178015_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178015_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:57:24.43 +50:20:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.324 211569852780732288 089.35236411573 +50.33418129791 14.5141 13.8996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178019_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178019_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 178021_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178021_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:03:13.13 +53:12:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.192 972613524777640192 090.80463627568 +53.20332989335 14.2866 13.6781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178022_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178022_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 178032_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178032_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 178034_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178034_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:46:11.52 +49:52:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.415 214126320393959808 086.54826760978 +49.87924206124 13.5846 12.8342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178036_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178036_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:01:55.64 +53:53:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.382 267127934816551680 075.48127764140 +53.88641075334 12.9738 12.0815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178038_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178038_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 178043_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178043_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:05:44.95 +55:47:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.237 997320822363767296 091.43736956149 +55.78991038628 12.6508 11.9243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178044_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178044_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 178046_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 178046_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 179174_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 179174_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 179228_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 179228_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 179455_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 179455_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 180307_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 180307_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 180331_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 180331_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 180342_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 180342_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 180737_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 180737_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 181868_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 181868_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 181872_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 181872_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 181913_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 181913_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:31:20.89 +49:56:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.456 213608377402547712 082.83696060179 +49.94089322860 12.6771 11.8623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182102_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 182102_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 182190_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 182190_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 182281_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 182281_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 182366_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 182366_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 182390_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 182390_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:00:08.24 +51:03:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.471 970522696042307200 090.03437989289 +51.05790024885 12.7697 11.8695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182784_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 182784_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 183217_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183217_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:47:45.46 +50:03:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.149 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183307_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183307_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:12:21.17 +54:45:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.538 997005739267042304 093.08857660385 +54.75575564760 13.2697 12.6498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183322_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183322_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 183335_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183335_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 183720_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183720_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:42:40.17 +49:46:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.247 214148619864314368 085.66689303923 +49.78234648811 13.6183 12.8648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183798_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183798_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:11:35.74 +52:39:14.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 183799_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183799_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 183875_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183875_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:22:37.79 +51:12:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.522 262108045758146048 080.65702308379 +51.20937134934 12.9621 11.9672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183885_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183885_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 183974_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183974_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:08:15.33 +54:54:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.972 996699319119851008 092.06420427911 +54.90939078022 13.4110 12.8023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183978_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 183978_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:19:01.66 +56:30:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.515 998044129216427392 094.75578843059 +56.50771081848 13.8774 13.3409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184006_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184006_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184086_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184086_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:17:44.07 +55:30:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.209 267530287349870336 079.43410487431 +55.51238583119 13.1166 12.1260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184180_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184180_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:56:20.15 +53:34:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.127 216137602038542464 089.08403325226 +53.57422793726 13.6574 13.1142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184236_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184236_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:01:04.87 +50:00:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.402 970368734350565760 090.26951411061 +50.00316418749 13.2862 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184246_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184246_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184268_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184268_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:25:00.71 +50:58:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.144 261894190746078080 081.25425538754 +50.97371673282 13.5754 12.9373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184326_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184326_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184474_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184474_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:51:23.20 +55:14:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.771 265213543334559488 087.84582725186 +55.24866331365 13.7181 13.1699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184657_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184657_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:34:00.25 +56:51:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.527 269204530025667968 083.49976764186 +56.86489304848 13.5024 12.8462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184673_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184673_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184680_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184680_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184691_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184691_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184724_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184724_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184835_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184835_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:54:40.84 +51:49:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.238 214932502935070208 088.66872391548 +51.81816212976 13.8431 13.2804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184880_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184880_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 184998_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 184998_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 185103_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185103_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:09:12.46 +56:23:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.130 997258764380573824 092.30195571984 +56.38409093408 13.6916 13.0101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185141_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185141_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 185176_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185176_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 185273_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185273_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 185314_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185314_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 185325_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185325_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 185395_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185395_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 185399_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185399_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:08:37.08 +55:33:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 4.673 997114698293065728 092.15379557460 +55.56720754847 14.3466 13.7389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185590_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185590_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:00:46.50 +56:55:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.422 997510694277846528 090.19419480859 +56.93089498721 13.5293 12.8014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185643_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185643_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:12:53.41 +49:59:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.240 261559114578625536 078.22273820517 +49.98715193918 13.4738 12.6620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185649_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185649_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:42:06.73 +54:48:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.276 264858160559896064 085.52797222088 +54.80217641092 13.6919 13.0786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185671_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185671_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 185672_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 185672_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:59:49.66 +54:19:15.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 186075_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186075_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:13:11.99 +53:10:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.103 996435131388354816 093.30089759080 +53.17787779392 13.9599 13.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186208_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186208_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186358_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186358_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186375_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186375_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:26:48.57 +51:22:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 0.991 262008814833767040 081.70193380999 +51.38031036299 13.8591 13.0607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186418_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186418_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:55:38.76 +52:59:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.233 215850938741053312 088.91089142227 +52.99729232081 14.2874 13.6077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186465_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186465_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186467_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186467_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186484_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186484_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186651_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186651_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:38:39.52 +50:23:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.234 215091829042420352 084.66477998579 +50.39127962753 13.6155 12.8000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186800_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186800_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186805_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186805_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186819_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186819_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:47:49.37 +51:04:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186849_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186849_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 186900_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 186900_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:52:56.37 +50:17:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.465 211522779938192640 088.23432783568 +50.28932790372 14.3115 13.6361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187119_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187119_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187153_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187153_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187353_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
Preparing report for the candidate 187353_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
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Considering the candidate 187406_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187406_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187430_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187430_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:59:01.76 +55:42:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.068 264584558258926592 089.75739332933 +55.71299024296 14.7375 14.0657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187609_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187609_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187676_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187676_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187726_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187726_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187778_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187778_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187930_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187930_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 187957_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 187957_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 188378_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 188378_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 188456_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
Preparing report for the candidate 188456_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
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Considering the candidate 188491_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
Preparing report for the candidate 188491_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
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Considering the candidate 188505_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
Preparing report for the candidate 188505_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
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Considering the candidate 188523_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 188523_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 98888_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 98888_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:11:45.01 +54:17:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121974_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 121974_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 06:19:47.91 +57:15:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133856_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 133856_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
**** FOUND 05:19:56.93 +56:05:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27904_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 27904_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 129803_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 129803_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56837_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
Preparing report for the candidate 56837_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
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Considering the candidate 91864_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103
The candidate 91864_fd_Aur-01-Q2b1x1_2026-03-26_22-40-40_20.00sec_-10.00C_LIGHT_0103 did not pass the final checks