This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
XX Gem,2461121.7572,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
XX Gem 20260322.2572 10.34CV 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:26:13.97 +33:22:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7572,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2572 12.75CV 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:32:30.92 +28:25:57.2 ;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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7572,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2572 13.81CV 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:38:33.32 +24:59:37.9 ;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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7572,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2572 13.85CV 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:55.99 +25:24:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2572 2461121.7572 13.88 07:44:58.22 +28:01:30.3
192.20279 23.33399 galactic Gem Second-epoch detections are separated by 0.5" and 6.9 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 J116.2534+28.0235 | 07:44:58.22 +28:01:30.3 (user input) | dubious (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 J116.2534+28.0235,2461121.7572,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J116.2534+28.0235 20260322.2572 13.88CV 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:44:58.22 +28:01:30.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7572,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2572 14.33CV 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:13.98 +34:25:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7572,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2572 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:57:52.05 +33:20:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7572,14.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2572 14.90CV 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:09:01.99 +24:52:10.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20_00sec_-14_90C_LIGHT_0099_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: 2461032.90042990 23.12.2025 09:36:27.143 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
First image: 2461032.90042990 23.12.2025 09:36:27.143 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Last image: 2461121.75749258 22.03.2026 06:10:37.359 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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): 15473
Objects passed selection criteria: 15467
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 15050.5
Average stars matched: 14791 (98.2758 %)
Memory usage VmPeak: 120168 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 Sun Mar 22 01:15:19 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90042990 23.12.2025 09:36:27.143 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
First image: 2461032.90042990 23.12.2025 09:36:27.143 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Last image: 2461121.75749258 22.03.2026 06:10:37.359 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 102
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 58 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): 87371
Objects passed selection criteria: 87215
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 84757.5
Average stars matched: 81972.2 (96.7139 %)
Memory usage VmPeak: 1875524 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 Sun Mar 22 01:17:37 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat to cache
SExtractor catalog cache: saved Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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: 2461121.75689594
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits exists and is non-empty
Saving wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits to local_wcs_cache/
'wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> 'local_wcs_cache/wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits'
wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits exists and is non-empty
Saving wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits to local_wcs_cache/
'wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> 'local_wcs_cache/wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits'
wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
Saving wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits to local_wcs_cache/
'wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits' -> 'local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits'
wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits exists and is non-empty
Saving wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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 08:00:00.612 +29:59:57.49
Second-epoch image center 08:00:01.162 +29:59:54.68
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:00:00.612 +29:59:57.49
Second-epoch image center 08:00:01.654 +30:00:34.91
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 08:00:01.162 +29:59:54.68
Second-epoch second image center 08:00:01.654 +30:00:34.91
Angular distance between the image centers 0.01132 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits &> /tmp/tmp.NoRxop9Pnn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits &> /tmp/tmp.cm1579Hyvv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.n1FIZqv1fX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.tR6oqaPzDc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
Found non-empty wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
The reference image (wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits) and catalog (wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat) found
'wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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 7809 out of 15844 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.959883
a=0.000000 b=1.000000 c=22.959883
From vast_summary.log: estimated ref. image limiting mag.: -7.51
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 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
2.2 pix Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
2.2 pix fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
2.2 pix fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
15.5 mag. Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
15.5 mag. Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
15.3 mag. fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
15.3 mag. fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.4 (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.NoRxop9Pnn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> 'wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1065, passed=15844
Got 15844 stars (including 14751 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
util/solve_plate_with_UCAC5 got 15844 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits -region wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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.cm1579Hyvv (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> 'wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1095, passed=15627
Got 15627 stars (including 14516 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat
util/solve_plate_with_UCAC5 got 15627 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits -region wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.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.n1FIZqv1fX (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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=922, passed=14652
Got 14652 stars (including 13711 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 14652 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.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.tR6oqaPzDc (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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=925, passed=14450
Got 14450 stars (including 13507 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 14450 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits'
Saving fully-calibrated image wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits'
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits'
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits'
Preparing the HTML report for the field Gem-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out02396.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20760_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 20760_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:34:52.08 +31:52:34.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20774_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 20774_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:11:01.34 +31:58:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20776_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 20776_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:20:06.25 +32:10:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20783_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 20783_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:53:52.88 +32:31:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02396_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 02396_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Gem-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:26:13.97 +33:22:16.7
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat to cache
SExtractor catalog cache: saved Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Creating symlink local_wcs_cache/wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits exists and is non-empty
wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits exists and is non-empty
wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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 08:00:00.612 +29:59:57.49
Second-epoch image center 08:00:01.162 +29:59:54.68
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:00:00.612 +29:59:57.49
Second-epoch image center 08:00:01.654 +30:00:34.91
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 08:00:01.162 +29:59:54.68
Second-epoch second image center 08:00:01.654 +30:00:34.91
Angular distance between the image centers 0.01132 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/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits &> /tmp/tmp.lmmqOVWxr1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits &> /tmp/tmp.bWcPInHuiN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.fGUFeam39l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.AnKKAJWjly
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
Found non-empty wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
The reference image (wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits) and catalog (wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat) found
'wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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 7869 out of 88194 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.864924
a=0.000000 b=1.000000 c=22.864924
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 74 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
2.1 pix Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
2.2 pix fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
2.1 pix fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
15.6 mag. Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
15.6 mag. Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
15.4 mag. fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
15.5 mag. fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.lmmqOVWxr1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> 'wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=6294, passed=88167
Got 88167 stars (including 81701 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
util/solve_plate_with_UCAC5 got 88167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits -region wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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.bWcPInHuiN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> 'wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=6271, passed=89775
Got 89775 stars (including 83346 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat
util/solve_plate_with_UCAC5 got 89775 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits -region wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.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.fGUFeam39l (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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=5373, passed=81011
Got 81011 stars (including 75502 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 81011 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.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.AnKKAJWjly (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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=5387, passed=82137
Got 82137 stars (including 76611 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 82137 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Saving fully-calibrated image wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-09-45_20.00sec_-14.90C_LIGHT_0099.fits
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.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_2026-03-22_CI_Gem-02-Q1b1x1_011126_TTUQ1b1x1_19373_E7mwyk6E/wcs_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100.fits
Preparing the HTML report for the field Gem-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out105603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out105687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106160.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 6s
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Considering the candidate 105603_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105603_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:05:10.57 +31:24:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.296 877876510551495168 121.29444162622 +31.41313564309 14.8945 14.4267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105604_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105604_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:52:39.29 +26:57:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.894 874240803556173696 118.16411289971 +26.95335516807 15.0376 14.4167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105610_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105610_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:51:38.98 +30:37:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.898 880534442473720576 117.91214619824 +30.62911021042 15.0581 14.6318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105611_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105611_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:43:15.33 +29:28:16.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)
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Considering the candidate 105613_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105613_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:54:20.53 +29:31:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.018 875875055791907840 118.58539196351 +29.53149891451 14.5845 13.7189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105619_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105619_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:48:05.83 +34:59:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 1.136 894583521016647552 117.02440805428 +34.98806036577 14.7358 14.2098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105621_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105621_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:57:11.60 +32:52:12.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)
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Considering the candidate 105626_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105626_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:42:43.21 +27:08:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 0.921 875182707063566080 115.67979630033 +27.13797764345 14.5281 14.0048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105627_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105627_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:12:01.26 +30:34:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.641 876793457238230272 123.00478060461 +30.57407208776 14.8481 14.0474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105630_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105630_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:07:44.79 +25:18:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.031 681119901193459584 121.93694092063 +25.31261716302 14.7551 14.1244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105631_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105631_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:12:09.20 +30:12:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 3.513 876766278685255168 123.03858029117 +30.21249215182 14.6027 14.0471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105632_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105632_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:09:46.98 +25:51:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105639_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105639_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:54:56.61 +32:06:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105642_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105642_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:48:12.95 +26:04:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105645_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105645_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:26:29.95 +34:51:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105687_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 105687_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 105700_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105700_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:33:32.51 +33:06:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105766_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105766_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:13:15.66 +29:33:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105781_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105781_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:33:33.81 +30:50:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105793_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 105793_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 105796_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 105796_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105806_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105806_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:43:38.29 +32:25:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105824_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 105824_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 105827_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105827_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:02:03.88 +33:43:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105866_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105866_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:33:23.84 +28:55:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105875_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105875_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:45:57.46 +27:52:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105883_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105883_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:46:05.63 +27:53:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105924_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 105924_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 105929_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105929_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:31:41.34 +26:02:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 0.363 871684816978237696 112.92215350832 +26.03710690659 14.5735 14.0814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105944_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105944_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:37:12.65 +33:40:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.710 892762867199775104 114.30267464008 +33.66796991621 14.7446 14.2822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105975_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105975_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:59:33.28 +25:54:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105979_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 105979_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 105990_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 105990_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:44:11.46 +33:20:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106004_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106004_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:02:44.71 +31:43:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 3.152 878084009012186240 120.68588626311 +31.72758401173 14.9368 14.2590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106010_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106010_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:48:52.80 +27:36:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.753 875093268665364224 117.22021455852 +27.61369817525 14.5188 14.0190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106012_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106012_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:39:26.93 +30:52:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106021_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106021_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:25:53.54 +31:09:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.033 892066356646685952 111.47292263052 +31.15800171946 14.7597 14.1843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106022_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106022_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:34:38.42 +30:30:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.094 707905859872702976 128.65974934887 +30.50762463969 14.7560 14.3007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106062_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106062_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:37:25.43 +32:53:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.749 892503622973055616 114.35651270500 +32.89027744996 14.8920 14.3870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106085_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106085_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:34:20.07 +34:26:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 1.288 711398973953362304 128.58323292985 +34.43690324588 15.0411 14.4542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106086_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106086_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:23:52.86 +34:03:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.219 893398694158122752 110.97031213819 +34.06008205173 14.8677 14.4829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106088_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106088_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:35:47.35 +30:43:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 0.170 879808833517429120 113.94728077318 +30.71825915708 14.7092 14.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106091_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106091_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:37:16.71 +25:18:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 2.051 868541347594304384 114.31899505929 +25.31217445673 14.8291 14.3442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106095_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106095_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:28:23.55 +33:43:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.586 903130093618097920 127.09759858900 +33.71858935615 14.8280 14.3624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106096_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106096_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:26:35.06 +30:15:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.496 885785022811728768 111.64645011017 +30.25795329827 15.0040 14.2686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106115_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106115_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:26:20.55 +33:18:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.263 893298806102178816 111.58569420273 +33.31084840577 14.8626 14.1403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106121_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106121_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:27:09.42 +25:13:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 2.207 870038676272625664 111.78883773039 +25.22754223207 14.6047 14.0210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106123_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106123_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:31:14.21 +26:59:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.554 872362421082145536 112.80885098646 +26.99151386330 14.8657 14.3546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106138_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106138_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:18:22.28 +29:27:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 2.359 708475303816203648 124.59209357977 +29.46610152827 14.6790 13.7938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106145_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106145_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:51:00.84 +27:31:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 0.565 875034376073889152 117.75333761615 +27.52285440616 14.8507 14.3881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106157_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106157_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:34:39.75 +29:03:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.631 879353498264713344 113.66513045242 +29.06110753741 14.6686 14.1833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106160_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 106160_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 106161_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106161_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:25:49.67 +25:51:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 5.037 871805419660193664 111.45722845167 +25.84873317487 14.8979 14.4596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106162_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106162_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:44:18.63 +24:59:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.455 867908097616570240 116.07727893627 +24.99735636411 14.8869 14.3007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106165_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106165_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:42:13.84 +25:16:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 2.313 868687994957681152 115.55789601521 +25.27844730028 15.0356 14.1956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106183_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106183_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:25:19.07 +28:58:19.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)
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Considering the candidate 106184_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106184_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:23:48.97 +33:14:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.092 893285891137261056 110.95419088186 +33.23561255913 15.1139 14.6344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106205_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106205_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:44:39.50 +33:02:54.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)
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Considering the candidate 106207_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106207_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:43:08.81 +30:56:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 0.664 880050515621258752 115.78659458070 +30.94873243970 15.0205 14.5488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106225_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106225_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:43:00.88 +28:51:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 2.369 878443686752923008 115.75378327054 +28.85182223034 14.8460 14.4554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106230_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106230_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:31:30.86 +33:47:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 3.665 893470780888969984 112.87744989776 +33.79805821724 15.0007 14.5070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106233_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106233_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:45:00.14 +26:26:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.663 874900304374090880 116.25097149720 +26.43836233560 15.0610 14.5732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106241_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106241_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:24:13.78 +30:41:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 3.122 886024510188592768 111.05641059984 +30.68380899630 14.9962 14.4824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106250_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106250_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 08:03:50.64 +29:15:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.615 876407116340232576 120.96151326837 +29.25383312835 15.0965 14.4450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106262_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106262_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:40:34.12 +25:56:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.183 868960879999624576 115.14191587592 +25.94370534925 14.9882 14.5423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106276_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106276_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:46:17.02 +33:31:21.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)
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Considering the candidate 106281_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106281_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:34:42.72 +32:22:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.754 892400406319089280 113.67776038376 +32.37614001386 14.7788 14.1693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106287_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106287_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:41:41.79 +30:22:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.231 879905762339309952 115.42400621819 +30.36953499433 14.9002 14.3795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106307_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106307_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:39:57.93 +28:36:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 1.315 878532953353944576 114.99109026327 +28.61368307662 15.0228 14.3802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106321_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106321_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:28:17.16 +26:16:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.974 871845448755262848 112.07090161660 +26.26814102488 14.8828 14.3836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106325_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106325_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:31:25.92 +26:30:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.997 871910972776852608 112.85804908945 +26.50711531668 14.7999 14.3489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106346_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106346_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:28:31.29 +25:14:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.384 871525525231092864 112.13028832980 +25.24520557529 14.6367 13.8255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106384_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 106384_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 07:34:18.13 +30:15:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.558 879678300871282560 113.57505137907 +30.25541043462 14.9790 14.3023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13030_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100
The candidate 13030_fd_Gem-02-Q1b1x1_2026-03-22_01-10-37_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
