This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh
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,2461118.8211,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
XX Gem 20260319.3211 10.15CV 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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:26:14.46 +33:22:16.1 ;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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3211 2461118.8211 13.96 07:25:55.51 +34:47:43.4
183.84115 21.70141 galactic Gem Second-epoch detections are separated by 5.6" and 5.0 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 | target | 07:25:55.51 +34:47:43.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
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
target,2461118.8211,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3211 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:25:55.51 +34:47:43.4 ;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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3211 2461118.8211 13.78 07:24:49.08 +33:53:49.1
184.67428 21.19338 galactic Gem Second-epoch detections are separated by 1.4" and 4.1 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 | target | 07:24:49.08 +33:53:49.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
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
target,2461118.8211,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3211 13.78CV 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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:24:49.08 +33:53:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3211 2461118.8211 13.22 07:24:54.89 +34:46:58.2
183.78208 21.50098 galactic Gem Second-epoch detections are separated by 6.8" and 3.0 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 | Gaia DR3 896808829472041856 | 07:24:54.51 +34:47:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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
Gaia DR3 896808829472041856,2461118.8211,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 896808829472041856 20260319.3211 13.22CV 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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:24:54.89 +34:46:58.2 ;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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8211,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3211 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:30:07.63 +28:47:50.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8211,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3211 13.43CV 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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:16.83 +25:28:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8211,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3211 13.57CV 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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:33.84 +25:06:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8211,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3211 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:44:44.68 +34:38:05.2 ;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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Last image: 2461118.82139353 19.03.2026 07:42:38.401 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 14909
Objects passed selection criteria: 14895
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 13893.8
Average stars matched: 13694.5 (98.5659 %)
Memory usage VmPeak: 120164 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:50:24 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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Last image: 2461118.82139353 19.03.2026 07:42:38.401 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.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: 34 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): 83090
Objects passed selection criteria: 82921
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 75834.2
Average stars matched: 73639.8 (97.1062 %)
Memory usage VmPeak: 1939864 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:51:55 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
SExtractor catalog cache: saved Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat to cache
SExtractor catalog cache: saved Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461118.82085888
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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits exists and is non-empty
Saving wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits to local_wcs_cache/
'wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> 'local_wcs_cache/wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits'
wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits exists and is non-empty
Saving wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits to local_wcs_cache/
'wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> 'local_wcs_cache/wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits'
wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits exists and is non-empty
Saving wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits to local_wcs_cache/
'wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits'
wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.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 08:00:06.128 +30:01:43.11
Angular distance between the image centers 0.04 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 08:00:04.602 +30:01:54.71
Angular distance between the image centers 0.04 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 08:00:06.128 +30:01:43.11
Second-epoch second image center 08:00:04.602 +30:01:54.71
Angular distance between the image centers 0.00638 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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits &> /tmp/tmp.yw150giZ1n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits &> /tmp/tmp.TV2Zg3H5ag
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits &> /tmp/tmp.234zgfFvQT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.qAj1yUsUhZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
Found non-empty wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
The reference image (wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits) and catalog (wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat) found
'wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
2.2 pix Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
2.5 pix fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
2.5 pix fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Limiting magnitude estimates:
15.5 mag. Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
15.5 mag. Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
15.0 mag. fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
15.0 mag. fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yw150giZ1n (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> 'wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS-calibrated image found: wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Checking if the catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS catalog name: wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits -region wcs_Gem-02-Q2b1x1_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-Q2b1x1_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.TV2Zg3H5ag (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> 'wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Checking if the catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS catalog name: wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits -region wcs_Gem-02-Q2b1x1_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-Q2b1x1_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.234zgfFvQT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=659, passed=12221
Got 12221 stars (including 11552 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 12221 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits -region wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.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.qAj1yUsUhZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=656, passed=12209
Got 12209 stars (including 11540 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 12209 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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: 0.49"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits'
Saving fully-calibrated image wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits'
Saving fully-calibrated image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits'
Preparing the HTML report for the field Gem-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02396.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 20754_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 20754_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:24:36.60 +27:53:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.913 707143687859094784 126.15278440327 +27.89597882015 12.4586 11.7947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20763_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 20763_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:34:52.09 +31:52:34.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20771_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 20771_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:04:31.99 +28:06:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.698 876011601392502656 121.13287111536 +28.10290240484 12.7426 12.0947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20780_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 20780_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:25:34.88 +33:42:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.738 903094904950192512 126.39554993442 +33.70556990404 12.4938 11.9642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02396_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 02396_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Gem-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:26:14.46 +33:22:16.1
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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
SExtractor catalog cache: saved Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat to cache
SExtractor catalog cache: saved Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Creating symlink local_wcs_cache/wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits exists and is non-empty
wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits exists and is non-empty
wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.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 08:00:06.128 +30:01:43.11
Angular distance between the image centers 0.04 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 08:00:04.602 +30:01:54.71
Angular distance between the image centers 0.04 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 08:00:06.128 +30:01:43.11
Second-epoch second image center 08:00:04.602 +30:01:54.71
Angular distance between the image centers 0.00638 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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits &> /tmp/tmp.r4CicHQBkO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits &> /tmp/tmp.vCa34HbCJ3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits &> /tmp/tmp.QZYSPOAhbf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.LypiNCDCYO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
Found non-empty wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits and wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat
The reference image (wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits) and catalog (wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat) found
'wcs_Gem-02-Q2b1x1_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 61 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
2.1 pix Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
2.4 pix fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
2.4 pix fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Limiting magnitude estimates:
15.6 mag. Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
15.6 mag. Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
15.1 mag. fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
15.1 mag. fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.r4CicHQBkO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits' -> 'wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS-calibrated image found: wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Checking if the catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
WCS catalog name: wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits -region wcs_Gem-02-Q2b1x1_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-Q2b1x1_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.vCa34HbCJ3 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits' -> 'wcs_Gem-02-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Checking if the catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits.cat corresponding to the image wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
WCS catalog name: wcs_Gem-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits -region wcs_Gem-02-Q2b1x1_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-Q2b1x1_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.QZYSPOAhbf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=3878, passed=63535
Got 63535 stars (including 59595 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 63535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 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-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits -region wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.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.LypiNCDCYO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3841, passed=63898
Got 63898 stars (including 59991 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 63898 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.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-Q2b1x1_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_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits
Saving fully-calibrated image wcs_Gem-02-Q2b1x1_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_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_Gem-02-Q2b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits
Saving fully-calibrated image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits
Saving fully-calibrated image wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits
Preparing the HTML report for the field Gem-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out105587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105623.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__out105639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out105613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105929.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 105587_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105587_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:18:44.11 +25:01:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 5.462 679320825292868736 124.68213166905 +25.02897598818 14.1920 13.6555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105590_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105590_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:26:44.86 +34:44:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 3.833 893819772751600000 111.68820965145 +34.73998896877 13.5781 12.9841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105592_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105592_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:26:05.98 +33:05:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.181 893106979979471616 111.52459766213 +33.08757933639 13.8497 13.1276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105595_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105595_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:29:20.23 +30:56:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 3.724 708902017406818816 127.33308562991 +30.94013189682 14.4914 14.0422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105596_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105596_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:24:35.37 +32:37:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 2.358 892974282670026880 111.14680948482 +32.63188369348 13.6180 13.1599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105597_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105597_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:25:35.21 +32:24:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.470 892955728411367296 111.39744967015 +32.40871863026 13.3838 12.9088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105602_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105602_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:26:22.27 +34:36:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 4.354 893811595133885056 111.59141184955 +34.61088832530 13.3981 12.6500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105606_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105606_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:24:23.55 +30:37:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 5.125 885977162469031552 111.09956507982 +30.63183992351 13.7805 13.3461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105610_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105610_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:24:46.71 +31:34:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.349 892842508776638720 111.19500980366 +31.58112387012 13.3707 12.8326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105612_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105612_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:29:59.49 +25:29:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.690 871558991616196096 112.49741921253 +25.48803186011 13.6388 13.2287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105613_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 105613_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105617_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105617_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:24:29.57 +31:11:17.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)
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Considering the candidate 105619_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105619_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:25:51.27 +25:52:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.928 871805900696525440 111.46392574904 +25.87862880564 13.3504 12.7316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105623_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105623_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:29:41.99 +34:54:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.489 893905362860348800 112.42681250769 +34.91288774589 12.9994 12.2739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105627_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105627_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:48:13.24 +26:04:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.765 874078522512554368 117.05537789275 +26.06976545977 13.8336 13.3175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105630_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105630_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:23:39.76 +33:35:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.517 893347120190880512 110.91516249652 +33.58821885171 13.0378 12.4514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105639_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105639_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:59:30.89 +25:10:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.330 681633922879854464 119.87911540533 +25.18086034032 13.8769 13.4135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105643_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105643_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:05:31.34 +25:08:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.844 681771533631779584 121.38084207619 +25.14228858990 13.8688 13.3665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105651_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 105651_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105660_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105660_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:24:45.24 +34:25:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.157 896783162747641344 111.18746460907 +34.43168964977 12.6357 11.9843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105663_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105663_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:26:37.84 +33:49:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.363 893702468605181696 111.65936467814 +33.82806277368 12.7695 12.2037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105665_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 105665_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105672_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105672_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:24:24.32 +33:57:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.774 893393295383452288 111.09981658362 +33.95097420965 12.1511 11.4043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105677_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105677_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 105680_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105680_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:47:51.11 +26:10:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.980 874083092357661824 116.96304309150 +26.17457243371 12.8726 12.3214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105685_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105685_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:23:44.57 +34:50:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 4.844 896859265271606016 110.93468108683 +34.84707644807 11.1852 10.5211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105692_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105692_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:34:52.11 +31:52:34.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 105700_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105700_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:43:57.71 +25:46:40.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105715_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 105715_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105763_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105763_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:32:14.15 +27:05:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.667 872322911680238208 113.05916647174 +27.08916875973 13.1309 12.6580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105764_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 105764_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105775_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105775_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:35:34.51 +27:12:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.369 872149738598014336 113.89306134641 +27.21139436403 13.3496 12.7266 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 105777_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105777_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:53:12.09 +27:54:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.837 875441710771776768 118.30029071497 +27.90135627911 13.4613 12.9670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105814_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105814_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:32:47.28 +28:58:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.425 873402185421219968 113.19659844043 +28.97379004769 13.5517 12.8179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105818_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 105818_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105830_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105830_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:33:33.77 +30:50:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.952 879846697949042048 113.39087433570 +30.83608281636 13.6356 12.9612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105833_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105833_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:21:47.60 +26:56:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.689 682975705022511360 125.44856588978 +26.94346797094 13.6530 13.0640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105841_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105841_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:44:57.69 +28:01:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 3.246 875341655212114048 116.23942763856 +28.02485756537 13.9382 13.2245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105864_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105864_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:53:34.73 +30:36:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.166 880508707029783424 118.39462652269 +30.61237181262 14.0856 13.6316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105866_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105866_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:53:10.66 +32:11:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.898 880936588850528512 118.29379756677 +32.18457947123 14.1471 13.6594 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 105872_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105872_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:47:04.32 +27:27:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.048 875250155230744320 116.76822632109 +27.45451648296 14.1743 13.7839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105881_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105881_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:43:38.04 +32:25:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.352 881882134491430784 115.90949537974 +32.43098772280 14.0631 13.5788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105882_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105882_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:35:01.82 +32:55:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.747 710691438220863616 128.75814905565 +32.92276177392 14.0051 13.2846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105887_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105887_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:59:21.93 +27:05:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.052 874477439074563328 119.84197355877 +27.09954744175 14.1662 13.6892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105893_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105893_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:04:07.56 +26:58:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.755 682275109957558272 121.03200059961 +26.97680369049 14.3824 13.9378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105905_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105905_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:51:09.45 +32:59:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 2.157 881785617985566720 117.78866185672 +32.98825824039 14.2387 13.7756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105908_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105908_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:43:54.43 +29:02:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.403 878475744388781056 115.97701980663 +29.03827620333 14.5964 14.1489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105919_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105919_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:43:11.44 +31:15:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.244 880105151901351808 115.79777380522 +31.25119438252 14.2200 13.6706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105922_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105922_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:33:56.62 +30:14:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.667 879677373158356480 113.48633307824 +30.23795838966 14.3622 13.8025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105929_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 105929_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105934_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105934_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:41:37.07 +30:47:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.084 879998533632783104 115.40410958924 +30.79597400602 14.4873 13.9332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105935_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105935_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:49:03.48 +28:28:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 2.131 875700920638838016 117.26510801737 +28.46819013169 14.4573 14.0386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105960_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105960_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:46:05.72 +27:53:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.696 875327327202999296 116.52362804780 +27.89131666035 14.5626 14.0585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105961_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105961_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:48:52.75 +27:36:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.526 875093268665364224 117.22021455852 +27.61369817525 14.5188 14.0190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105979_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105979_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:54:53.44 +30:47:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.595 880505099257191552 118.72254353646 +30.79290461667 14.3633 13.8186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105994_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 105994_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 08:06:00.03 +32:25:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 4.300 902148264095259008 121.50139831073 +32.41834003577 14.5934 14.0732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106027_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 106027_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:45:57.39 +27:52:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.800 875327017965373184 116.48950733325 +27.86924250004 14.4468 13.9262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 11308_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 11308_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 71229_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 71229_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:26:54.14 +26:16:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.924 871854176128848128 111.72470901419 +26.26815692599 13.4639 13.0099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13030_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 13030_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 07:26:14.46 +33:22:16.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 101162_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041
The candidate 101162_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks