This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.9766,7.29,0.05,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 20260817.4766 7.29CV 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
Mean magnitude and position on the discovery images:
2026 08 17.4766 2461269.9766 9.02 06:06:04.92 +22:27:21.2
187.91804 0.71380 galactic Gem Second-epoch detections are separated by 1.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1 Ceres 1 -0 1 8.9 -0 -0
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:06:04.92 +22:27:21.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:06:04.92 +22:27:21.2: 99.00 +/- 99.00 bad_region
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.9766,9.02,0.05,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 20260817.4766 9.02CV 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
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.9766,7.99,0.05,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 20260817.4766 7.99CV 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
Mean magnitude and position on the discovery images:
2026 08 17.4766 2461269.9766 11.19 06:23:22.43 +22:51:11.0
189.46945 4.41120 galactic Gem Second-epoch detections are separated by 0.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.27 Euterpe -0 -0 1 11.5 0 0
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:23:22.43 +22:51:11.0: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:23:22.43 +22:51:11.0: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.9766,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.4766 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.4766 2461269.9766 12.18 06:29:20.88 +24:34:05.5
188.56828 6.41286 galactic Gem Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.30 Urania 0 0 0 12.4 0 0
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:20.88 +24:34:05.5: 15.72 +/- 0.31 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:20.88 +24:34:05.5: 15.25 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.9766,12.18,0.05,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 20260817.4766 12.18CV 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
Mean magnitude and position on the discovery images:
2026 08 17.4766 2461269.9766 12.95 06:16:24.15 +19:31:58.4
191.64022 1.41722 galactic Ori Second-epoch detections are separated by 1.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.712 Boliviana -1 0 1 13.3 -0 0
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:16:24.15 +19:31:58.4: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:16:24.15 +19:31:58.4: 15.65 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.65 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!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!
TCP 2026 08 17.4766* 06 16 24.15 +19 31 58.4 12.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.9766,12.95,0.05,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 20260817.4766 12.95CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
First image: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Last image: 2461269.97689434 17.08.2026 11:26:33.671 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 16644
Objects passed selection criteria: 16551
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 13171.2
Average stars matched: 11015 (83.6291 %)
Memory usage VmPeak: 248312 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 06:45:07 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: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
First image: 2461058.61760534 18.01.2026 02:49:11.101 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Last image: 2461269.97689434 17.08.2026 11:26:33.671 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 51
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 21 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 121212
Objects passed selection criteria: 120871
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 97936
Average stars matched: 86685.8 (88.5127 %)
Memory usage VmPeak: 622932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 06:46:12 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
SExtractor catalog cache: saved Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.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: 2461269.97629854
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits exists and is non-empty
wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits exists and is non-empty
wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (1st reference image)
verification OK: wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:40.095 +22:00:29.68 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits (1st new image)
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Image size: 937.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:27:30.966 +21:58:12.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:27:40.095 +22:00:29.68
Second-epoch image center 06:27:30.966 +21:58:12.22
Angular distance between the image centers 0.0520 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits (2nd new image)
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Image size: 937.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:27:33.718 +21:58:38.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:27:40.095 +22:00:29.68
Second-epoch image center 06:27:33.718 +21:58:38.58
Angular distance between the image centers 0.0395 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 06:27:30.966 +21:58:12.22
Second-epoch second image center 06:27:33.718 +21:58:38.58
Angular distance between the image centers 0.01291 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits &> /tmp/tmp.JpW7D4E73j
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.hP6YOQug0M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits &> /tmp/tmp.UjPKpnbIvY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits &> /tmp/tmp.RSEtknmRgF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
Found non-empty wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
The reference image (wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits) and catalog (wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat) found
'wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat' -> 'wcsmag.cat'
Read 29338 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9455 to 105.5063 deg, Dec +16.3282 to +27.3630 deg
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
Tycho-2 catalog search boundaries: RA 87.9455 to 105.5063 deg, Dec 16.3282 to 27.3630 deg
Loaded 19945 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14221 out of 15960 total matches.
Matched with Tycho-2 15960 out of 29338 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881900
a=0.000000 b=1.000000 c=22.881900
From vast_summary.log: estimated ref. image limiting mag.: -7.79
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29338 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9455 to 105.5063 deg, Dec +16.3282 to +27.3630 deg
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
Tycho-2 catalog search boundaries: RA 87.9455 to 105.5063 deg, Dec 16.3282 to 27.3630 deg
Loaded 19945 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14221 out of 15960 total matches.
Matched with Tycho-2 15960 out of 29338 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Forced-photometry filter: calibrated wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (aperture=6.2)
Read 31529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 88.2224 to 105.7491 deg, Dec +16.5172 to +27.2358 deg
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
Tycho-2 catalog search boundaries: RA 88.2224 to 105.7491 deg, Dec 16.5172 to 27.2358 deg
Loaded 19341 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14457 out of 15956 total matches.
Matched with Tycho-2 15956 out of 31529 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Forced-photometry filter: calibrated wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
2.5 pix Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
2.4 pix fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
2.5 pix fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Limiting magnitude estimates:
15.1 mag. Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
15.1 mag. Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
13.0 mag. fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
13.0 mag. fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.JpW7D4E73j (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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits' -> 'wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Checking if the catalog wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS catalog name: wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3278, bad_region=6704, passed=29338
Got 29338 stars (including 19960 good ones) from the SExtractor catalog wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 29338 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 4803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 24050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 24050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 24050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4804 stars left (next iteration limit 5282)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits N_match=4804 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.324 n_q1=1455 n_q2=895 n_q3=1550 n_q4=904 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits -region wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hP6YOQug0M (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_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_Gem-03-Q2b1x1_2026-03-21_23-25-36_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/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3030, bad_region=7092, passed=31529
Got 31529 stars (including 22011 good ones) from the SExtractor catalog wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat
util/solve_plate_with_UCAC5 got 31529 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 26103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4827 matched stars entering correct_measured_positions(), 26103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4827 matched stars entering correct_measured_positions(), 26103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4827 stars left (next iteration limit 5306)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits N_match=4827 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.486 sigma_q4_arcsec=0.427 n_q1=1500 n_q2=1011 n_q3=1428 n_q4=888 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UjPKpnbIvY (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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Checking if the catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
WCS catalog name: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=995, bad_region=830, passed=3945
Got 3945 stars (including 2329 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat
util/solve_plate_with_UCAC5 got 3945 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 2270 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2243 matched stars entering correct_measured_positions(), 2242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2243 matched stars entering correct_measured_positions(), 3230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 2272 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2244 matched stars entering correct_measured_positions(), 3230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 2244 matched stars entering correct_measured_positions(), 3230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 2244 stars left (next iteration limit 2467)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2244 robust_rms=6.034 arcsec worst_quadrant_rms=12.228 arcsec
SIP_REFIT: SIP order 3 trial: matched=2244 robust_rms=0.736 arcsec worst_quadrant_rms=0.927 arcsec
SIP_REFIT: SIP order 5 trial: matched=2244 robust_rms=0.495 arcsec worst_quadrant_rms=0.593 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2244 robust_rms_before=1.061 arcsec robust_rms_before_corrected=0.572 arcsec robust_rms_after=0.495 arcsec worst_quadrant_rms_before=0.666 worst_quadrant_rms_after=0.593
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Image size: 937.7'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:27:30.919 +21:58:11.64 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3945 stars ###
'wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/correct_sextractor_wcs_catalog_usingxy2sky2560506.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.061 -> 0.495 arcsec)
WCS_QUALITY_DIAG: file=fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits N_match=2244 sigma_overall_arcsec=0.523 sigma_q1_arcsec=0.476 sigma_q2_arcsec=0.469 sigma_q3_arcsec=0.633 sigma_q4_arcsec=0.503 n_q1=717 n_q2=397 n_q3=741 n_q4=389 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits -region wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RSEtknmRgF (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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Checking if the catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
WCS catalog name: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1340, bad_region=759, passed=3543
Got 3543 stars (including 1767 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat
util/solve_plate_with_UCAC5 got 3543 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 1724 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1703 matched stars entering correct_measured_positions(), 1701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1703 matched stars entering correct_measured_positions(), 2844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 1726 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1704 matched stars entering correct_measured_positions(), 2844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 1704 matched stars entering correct_measured_positions(), 2844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 1704 stars left (next iteration limit 1873)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1704 robust_rms=5.598 arcsec worst_quadrant_rms=17.432 arcsec
SIP_REFIT: SIP order 3 trial: matched=1704 robust_rms=0.875 arcsec worst_quadrant_rms=1.056 arcsec
SIP_REFIT: SIP order 5 trial: matched=1704 robust_rms=0.608 arcsec worst_quadrant_rms=0.699 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1704 robust_rms_before=1.205 arcsec robust_rms_before_corrected=0.691 arcsec robust_rms_after=0.608 arcsec worst_quadrant_rms_before=0.792 worst_quadrant_rms_after=0.699
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Image size: 937.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:27:33.676 +21:58:38.05 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3543 stars ###
'wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/correct_sextractor_wcs_catalog_usingxy2sky2560457.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.205 -> 0.608 arcsec)
WCS_QUALITY_DIAG: file=fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits N_match=1704 sigma_overall_arcsec=0.626 sigma_q1_arcsec=0.525 sigma_q2_arcsec=0.602 sigma_q3_arcsec=0.794 sigma_q4_arcsec=0.586 n_q1=558 n_q2=289 n_q3=577 n_q4=280 worst_quadrant_to_overall_ratio=1.268
The image catalog is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits -region wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits to local_wcs_cache/
'wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits'
Saving the final (post-refit) wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits'
Saving the final (post-refit) wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits to local_wcs_cache/
'wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits' -> 'local_wcs_cache/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits'
Saving the final (post-refit) wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits to local_wcs_cache/
'wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits' -> 'local_wcs_cache/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits sigma_overall=0.382 worst_q_ratio=1.117
ref2=Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits sigma_overall=0.434 worst_q_ratio=1.119
new1=fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits sigma_overall=0.523 worst_q_ratio=1.210
new2=fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits sigma_overall=0.626 worst_q_ratio=1.268
reference average sigma_overall=0.408 worst_q_ratio=1.118
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057_astrometric_residuals.png (4804 matched stars from wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041_astrometric_residuals.png (4827 matched stars from wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564_astrometric_residuals.png (2244 matched stars from wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565_astrometric_residuals.png (1704 matched stars from wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits'
Saving fully-calibrated image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits'
Preparing the HTML report for the field Gem-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:06:04.92 +22:27:21.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:06:04.92 +22:27:21.2: 99.00 +/- 99.00 bad_region
Adding exclusion_list_local.txt__out38612.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38608_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
Preparing report for the candidate 38608_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38612_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
Preparing report for the candidate 38612_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Gem-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:06:04.92 +22:27:21.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
SExtractor catalog cache: saved Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits exists and is non-empty
wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits exists and is non-empty
wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (1st reference image)
verification OK: wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:27:40.095 +22:00:29.68 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits (1st new image)
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Image size: 937.7'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:27:30.919 +21:58:11.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:27:40.095 +22:00:29.68
Second-epoch image center 06:27:30.919 +21:58:11.64
Angular distance between the image centers 0.0522 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits (2nd new image)
verification OK: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Image size: 937.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:27:33.676 +21:58:38.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:27:40.095 +22:00:29.68
Second-epoch image center 06:27:33.676 +21:58:38.05
Angular distance between the image centers 0.0397 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 06:27:30.919 +21:58:11.64
Second-epoch second image center 06:27:33.676 +21:58:38.05
Angular distance between the image centers 0.01294 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits &> /tmp/tmp.BrtIm2zr6E
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.TtqR6veNEV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits &> /tmp/tmp.T4anLgsEqv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits &> /tmp/tmp.44ny9Tu1fZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
Found non-empty wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits and wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
The reference image (wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits) and catalog (wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat) found
'wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat' -> 'wcsmag.cat'
Read 206292 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9318 to 105.5265 deg, Dec +16.3091 to +27.3656 deg
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
Tycho-2 catalog search boundaries: RA 87.9318 to 105.5265 deg, Dec 16.3091 to 27.3656 deg
Loaded 20018 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 11191 out of 16872 total matches.
Matched with Tycho-2 16872 out of 206292 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.723200
a=0.000000 b=1.000000 c=22.723200
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 206292 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.9318 to 105.5265 deg, Dec +16.3091 to +27.3656 deg
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
Tycho-2 catalog search boundaries: RA 87.9318 to 105.5265 deg, Dec 16.3091 to 27.3656 deg
Loaded 20018 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 11191 out of 16872 total matches.
Matched with Tycho-2 16872 out of 206292 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Forced-photometry filter: calibrated wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (aperture=4.6)
Read 188638 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 88.2221 to 105.7490 deg, Dec +16.4980 to +27.2397 deg
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
Tycho-2 catalog search boundaries: RA 88.2221 to 105.7490 deg, Dec 16.4980 to 27.2397 deg
Loaded 19379 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 11515 out of 16583 total matches.
Matched with Tycho-2 16583 out of 188638 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Forced-photometry filter: calibrated wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 40 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
2.4 pix Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
2.1 pix fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
2.0 pix fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Limiting magnitude estimates:
15.3 mag. Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
15.3 mag. Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
13.1 mag. fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
13.1 mag. fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BrtIm2zr6E (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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.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-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits' -> 'wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
Checking if the catalog wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits
WCS catalog name: wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=31903, bad_region=37736, passed=206254
Got 206254 stars (including 141027 good ones) from the SExtractor catalog wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 206254 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4828 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 4785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 177293 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4828 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 177293 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 177293 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4784 stars left (next iteration limit 5262)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits N_match=4784 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.424 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.299 n_q1=1462 n_q2=892 n_q3=1535 n_q4=895 worst_quadrant_to_overall_ratio=1.133
The image catalog is written to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits -region wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TtqR6veNEV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.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-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat corresponding to the image wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_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_Gem-03-Q2b1x1_2026-03-21_23-25-36_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/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=29566, bad_region=30361, passed=188602
Got 188602 stars (including 132646 good ones) from the SExtractor catalog wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat
util/solve_plate_with_UCAC5 got 188602 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 4804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 166604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4845 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 166604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 166604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4803 stars left (next iteration limit 5283)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits N_match=4803 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.434 sigma_q3_arcsec=0.497 sigma_q4_arcsec=0.399 n_q1=1499 n_q2=1022 n_q3=1389 n_q4=893 worst_quadrant_to_overall_ratio=1.134
The image catalog is written to wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.T4anLgsEqv (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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Checking if the catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
WCS catalog name: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=3, blended=1970, bad_region=6112, passed=39994
Got 39994 stars (including 32236 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat
util/solve_plate_with_UCAC5 got 39994 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 4812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 35511 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 35511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 35511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4811 stars left (next iteration limit 5292)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4811 robust_rms=6.400 arcsec worst_quadrant_rms=9.105 arcsec
SIP_REFIT: SIP order 3 trial: matched=4811 robust_rms=0.660 arcsec worst_quadrant_rms=0.872 arcsec
SIP_REFIT: SIP order 5 trial: matched=4811 robust_rms=0.483 arcsec worst_quadrant_rms=0.597 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4811 robust_rms_before=0.490 arcsec robust_rms_before_corrected=0.536 arcsec robust_rms_after=0.483 arcsec worst_quadrant_rms_before=0.594 worst_quadrant_rms_after=0.597
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.594 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits N_match=4811 sigma_overall_arcsec=0.540 sigma_q1_arcsec=0.518 sigma_q2_arcsec=0.507 sigma_q3_arcsec=0.640 sigma_q4_arcsec=0.481 n_q1=1518 n_q2=987 n_q3=1385 n_q4=921 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits -region wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.44ny9Tu1fZ (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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
WCS_IMAGE_NAME=wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
WCS-calibrated image found: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Checking if the catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat corresponding to the image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
WCS catalog name: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=6, blended=2155, bad_region=5891, passed=38875
Got 38875 stars (including 31229 good ones) from the SExtractor catalog wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat
util/solve_plate_with_UCAC5 got 38875 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 34610 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 34610 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 34610 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 4819 stars left (next iteration limit 5299)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4819 robust_rms=6.211 arcsec worst_quadrant_rms=9.443 arcsec
SIP_REFIT: SIP order 3 trial: matched=4819 robust_rms=0.747 arcsec worst_quadrant_rms=0.916 arcsec
SIP_REFIT: SIP order 5 trial: matched=4819 robust_rms=0.565 arcsec worst_quadrant_rms=0.656 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4819 robust_rms_before=0.603 arcsec robust_rms_before_corrected=0.622 arcsec robust_rms_after=0.565 arcsec worst_quadrant_rms_before=0.662 worst_quadrant_rms_after=0.656
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.662 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits N_match=4819 sigma_overall_arcsec=0.623 sigma_q1_arcsec=0.571 sigma_q2_arcsec=0.574 sigma_q3_arcsec=0.744 sigma_q4_arcsec=0.601 n_q1=1520 n_q2=985 n_q3=1395 n_q4=919 worst_quadrant_to_overall_ratio=1.195
The image catalog is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits -region wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-25-42_20.00sec_-0.00C_LIGHT_0564.fits
Saving fully-calibrated image wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.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_2026-08-17_CI_Gem-03-Q2b1x1_064234_TTUQ2b1x1_2534436_EnGhLTuR/wcs_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565.fits
Preparing the HTML report for the field Gem-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:58.99 +21:54:26.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:09.72 +19:32:33.1: 12.14 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:32:01.23 +26:06:15.2: 11.63 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:36:32.60 +21:38:00.1: 12.10 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:43:52.47 +23:55:57.2: 12.14 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:03:04.84 +24:48:40.8: 11.75 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:43:52.47 +23:55:57.2: 12.06 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:32:01.23 +26:06:15.2: 11.49 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:58.99 +21:54:26.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:09.72 +19:32:33.1: 12.03 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:36:32.60 +21:38:00.1: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.00
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter REJECTED candidate at 06:32:01.23 +26:06:15.2: ref_mag=11.55 +/- 0.00 new_mean_mag=11.8517 delta=-0.30 (need > 0.90)
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter REJECTED candidate at 06:27:09.72 +19:32:33.1: ref_mag=12.07 +/- 0.01 new_mean_mag=12.3553 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:27:58.99 +21:54:26.3: ref_mag=12.70 +/- 0.01 new_mean_mag=12.9539 delta=-0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:43:52.47 +23:55:57.2: ref_mag=12.10 +/- 0.01 new_mean_mag=12.3433 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:36:32.60 +21:38:00.1: ref_mag=12.05 +/- 0.01 new_mean_mag=12.7234 delta=-0.67 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:06:08.57 +25:14:37.2: 11.16 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:03:04.84 +24:48:40.8: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter REJECTED candidate at 06:03:04.84 +24:48:40.8: ref_mag=11.75 +/- 0.01 new_mean_mag=11.8884 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:28:55.61 +20:16:16.7: 11.62 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:06:08.57 +25:14:37.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 11.16 +/- 0.01
Forced photometry filter REJECTED candidate at 06:06:08.57 +25:14:37.2: ref_mag=11.16 +/- 0.01 new_mean_mag=11.4243 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:39:52.98 +19:18:39.3: 11.61 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:45:11.19 +22:06:08.6: 11.39 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:14.91 +25:21:39.4: 11.83 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:30:41.37 +20:24:34.9: 11.92 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:28:55.61 +20:16:16.7: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter REJECTED candidate at 06:28:55.61 +20:16:16.7: ref_mag=11.60 +/- 0.01 new_mean_mag=11.6273 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:42:15.64 +18:46:38.6: 11.89 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:14.14 +23:18:09.8: 12.20 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:45:11.19 +22:06:08.6: 11.22 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:39:52.98 +19:18:39.3: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Forced photometry filter REJECTED candidate at 06:45:11.19 +22:06:08.6: ref_mag=11.29 +/- 0.00 new_mean_mag=11.6052 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:39:52.98 +19:18:39.3: ref_mag=11.51 +/- 0.01 new_mean_mag=11.8610 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:14.91 +25:21:39.4: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter REJECTED candidate at 06:42:14.91 +25:21:39.4: ref_mag=11.81 +/- 0.01 new_mean_mag=11.8448 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:30:41.37 +20:24:34.9: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter REJECTED candidate at 06:30:41.37 +20:24:34.9: ref_mag=11.92 +/- 0.01 new_mean_mag=12.0193 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:27:57.66 +23:40:57.9: 12.17 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:01:14.14 +23:18:09.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:42:15.64 +18:46:38.6: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.02
Forced photometry filter REJECTED candidate at 06:01:14.14 +23:18:09.8: ref_mag=12.20 +/- 0.02 new_mean_mag=12.1776 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter REJECTED candidate at 06:42:15.64 +18:46:38.6: ref_mag=11.78 +/- 0.01 new_mean_mag=12.1856 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:41:29.92 +21:40:29.2: 12.19 +/- 0.01 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:27:57.66 +23:40:57.9: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 06:27:57.66 +23:40:57.9: ref_mag=12.17 +/- 0.01 new_mean_mag=12.1333 delta=0.04 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:38:49.54 +21:52:44.9: 12.51 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:41:29.92 +21:40:29.2: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 06:41:29.92 +21:40:29.2: ref_mag=12.09 +/- 0.01 new_mean_mag=12.3260 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:38:49.54 +21:52:44.9: 12.37 +/- 0.02 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:16:24.15 +19:31:58.4: 15.97 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter REJECTED candidate at 06:38:49.54 +21:52:44.9: ref_mag=12.43 +/- 0.01 new_mean_mag=12.5722 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:23:22.43 +22:51:11.0: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:02:36.65 +22:14:02.6: 10.33 +/- 0.00 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-01-17_20-49-11_20.00sec_-14.90C_LIGHT_0057.fits at 06:29:20.88 +24:34:05.5: 15.72 +/- 0.31 detection
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:16:24.15 +19:31:58.4: 15.65 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.65 +/- 0.28
Forced photometry filter KEPT candidate at 06:16:24.15 +19:31:58.4: ref_mag=15.65 +/- 0.28 new_mean_mag=12.9200 delta=2.73 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:23:22.43 +22:51:11.0: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:02:36.65 +22:14:02.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 10.33 +/- 0.00
Forced photometry filter REJECTED candidate at 06:02:36.65 +22:14:02.6: ref_mag=10.33 +/- 0.00 new_mean_mag=9.4503 delta=0.87 (need > 0.90)
Forced photometry on wcs_Gem-03-Q2b1x1_2026-03-21_23-25-36_20.00sec_-15.00C_LIGHT_0041.fits at 06:29:20.88 +24:34:05.5: 15.25 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.18
Forced photometry filter KEPT candidate at 06:29:20.88 +24:34:05.5: ref_mag=15.40 +/- 0.18 new_mean_mag=12.1753 delta=3.22 (need > 0.90)
Adding exclusion_list_local.txt__out121735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216761.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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: 2s
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Considering the candidate 261034_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261034_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261036_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261036_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:27:42.53 +21:10:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261039_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261039_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:23:45.91 +22:01:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261044_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261044_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261048_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261048_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:33:37.81 +23:30:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261053_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261053_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:42:45.78 +18:14:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261054_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261054_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261056_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261056_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:18:57.81 +23:16:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261059_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261059_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261063_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261063_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261066_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261066_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:28:53.31 +17:47:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261067_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261067_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261070_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261070_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:27:05.68 +24:56:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261071_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261071_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:43:01.99 +21:22:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261072_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261072_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:18:51.59 +18:25:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261074_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261074_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261077_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
Preparing report for the candidate 261077_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
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Considering the candidate 261080_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261080_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:06:04.96 +22:27:21.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 261102_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261102_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:14:39.80 +22:30:00.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 261104_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261104_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:14:36.49 +22:29:48.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 261114_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261114_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261119_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261119_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261126_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261126_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:29:01.49 +20:10:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261128_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261128_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261129_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261129_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:28:51.67 +24:02:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261135_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261135_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261149_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261149_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261158_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261158_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:15:04.25 +22:32:08.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 261162_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261162_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261170_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261170_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261176_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261176_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:39:40.63 +23:17:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261187_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261187_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261192_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261192_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:33:46.04 +21:04:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261196_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261196_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261202_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261202_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
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Considering the candidate 261221_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 261221_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
**** FOUND 06:18:10.88 +21:04:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121735_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
Preparing report for the candidate 121735_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
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Considering the candidate 153958_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
Preparing report for the candidate 153958_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
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Considering the candidate 216761_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
Preparing report for the candidate 216761_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
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Considering the candidate 116217_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565
The candidate 116217_fd_Gem-03-Q2b1x1_2026-08-17_06-26-33_20.00sec_0.00C_LIGHT_0565 did not pass the final checks
