This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT
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,2461186.6217,6.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.1217 6.89CV 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,2461186.6217,7.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.1217 7.01CV 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,2461186.6217,7.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.1217 7.40CV 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,2461186.6217,7.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.1217 7.36CV 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,2461186.6217,7.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.1217 7.41CV 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,2461186.6217,7.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.1217 7.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1217 2461186.6217 13.05 07:21:58.30 +26:27:31.8
191.83621 17.99922 galactic Gem Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.42 Isis 2 -2 2 13.6 -0 -0
Forced photometry on wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits at 07:21:58.30 +26:27:31.8: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits at 07:21:58.30 +26:27:31.8: 16.09 +/- 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,2461186.6217,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.1217 13.05CV 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: 2461058.73760365 18.01.2026 05:41:58.955 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
First image: 2461058.73760365 18.01.2026 05:41:58.955 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Last image: 2461186.62191372 26.05.2026 02:55:23.345 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 20662
Objects passed selection criteria: 20552
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 13829.8
Average stars matched: 13012.8 (94.0924 %)
Memory usage VmPeak: 125696 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 22:01:34 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: 2461058.73760365 18.01.2026 05:41:58.955 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
First image: 2461058.73760365 18.01.2026 05:41:58.955 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Last image: 2461186.62191372 26.05.2026 02:55:23.345 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 31
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 26 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 134724
Objects passed selection criteria: 134251
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 90868.2
Average stars matched: 86310 (94.9837 %)
Memory usage VmPeak: 1901860 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 22:05:27 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
SExtractor catalog cache: saved Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.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: 2461186.62140441
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits exists and is non-empty
Saving wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits to local_wcs_cache/
'wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits'
wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits exists and is non-empty
Saving wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits to local_wcs_cache/
'wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits' -> 'local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits'
wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits'
wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits (1st reference image)
verification OK: wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Image size: 941.6'x627.1' 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: 07:22:55.118 +21:59:39.20 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-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits (1st new image)
verification OK: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Image size: 941.6'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:23:10.851 +21:59:34.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:22:55.118 +21:59:39.20
Second-epoch image center 07:23:10.851 +21:59:34.32
Angular distance between the image centers 0.0608 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits (2nd new image)
verification OK: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Image size: 941.6'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:23:13.966 +21:59:36.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:22:55.118 +21:59:39.20
Second-epoch image center 07:23:13.966 +21:59:36.20
Angular distance between the image centers 0.0728 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 07:23:10.851 +21:59:34.32
Second-epoch second image center 07:23:13.966 +21:59:36.20
Angular distance between the image centers 0.01205 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits &> /tmp/tmp.Ww7JHLZBZk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.nba5q3doyO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits &> /tmp/tmp.D1iVvLPfMj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits &> /tmp/tmp.R9zKjrltkl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits and wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits and wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
Found non-empty wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits and wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
The reference image (wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits) and catalog (wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat) found
'wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat' -> 'wcsmag.cat'
Read 22550 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 101.7556 to 119.3352 deg, Dec +16.3006 to +27.3458 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 101.7556 to 119.3352 deg, Dec 16.3006 to 27.3458 deg
Loaded 14532 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): 10648 out of 11733 total matches.
Matched with Tycho-2 11733 out of 22550 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.904800
a=0.000000 b=1.000000 c=22.904800
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 22550 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 101.7556 to 119.3352 deg, Dec +16.3006 to +27.3458 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 101.7556 to 119.3352 deg, Dec 16.3006 to 27.3458 deg
Loaded 14532 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): 10648 out of 11733 total matches.
Matched with Tycho-2 11733 out of 22550 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits:
Forced-photometry filter: calibrated wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits -> calib.txt_param_ref_wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits (aperture=6.2)
Read 23656 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 102.0351 to 119.5904 deg, Dec +16.4807 to +27.2946 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 102.0351 to 119.5904 deg, Dec 16.4807 to 27.2946 deg
Loaded 13969 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): 10670 out of 11761 total matches.
Matched with Tycho-2 11761 out of 23656 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits:
Forced-photometry filter: calibrated wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits -> calib.txt_param_ref_wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
2.3 pix Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
3.2 pix fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
3.2 pix fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
2.1 pix wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
2.3 pix wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
Limiting magnitude estimates:
15.3 mag. Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
15.3 mag. Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
13.6 mag. fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
13.6 mag. fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Ww7JHLZBZk (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits' -> 'wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2218, passed=22550
Got 22550 stars (including 20300 good ones) from the SExtractor catalog wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 22550 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 22225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 22223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 22223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits N_match=953 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.402 sigma_q4_arcsec=0.325 n_q1=221 n_q2=247 n_q3=258 n_q4=227 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits -region wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nba5q3doyO (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.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-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits' -> 'wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2265, passed=23656
Got 23656 stars (including 21362 good ones) from the SExtractor catalog wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 23656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 22858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 22857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 22857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits N_match=950 sigma_overall_arcsec=0.413 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.379 sigma_q4_arcsec=0.362 n_q1=167 n_q2=275 n_q3=215 n_q4=293 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.D1iVvLPfMj (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=249, passed=4828
Got 4828 stars (including 4576 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 4828 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 4593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 4594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 4594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits N_match=940 sigma_overall_arcsec=0.462 sigma_q1_arcsec=0.424 sigma_q2_arcsec=0.552 sigma_q3_arcsec=0.454 sigma_q4_arcsec=0.498 n_q1=302 n_q2=227 n_q3=305 n_q4=106 worst_quadrant_to_overall_ratio=1.194
The image catalog is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits -region wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.R9zKjrltkl (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=242, passed=4646
Got 4646 stars (including 4402 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 4646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 4409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 4398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 942 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits N_match=942 sigma_overall_arcsec=0.485 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.566 sigma_q3_arcsec=0.480 sigma_q4_arcsec=0.527 n_q1=304 n_q2=220 n_q3=314 n_q4=104 worst_quadrant_to_overall_ratio=1.167
The image catalog is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits -region wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits sigma_overall=0.378 worst_q_ratio=1.064
ref2=Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits sigma_overall=0.413 worst_q_ratio=1.154
new1=fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits sigma_overall=0.462 worst_q_ratio=1.194
new2=fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits sigma_overall=0.485 worst_q_ratio=1.167
reference average sigma_overall=0.3955 worst_q_ratio=1.109
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229_astrometric_residuals.png (953 matched stars from wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153_astrometric_residuals.png (950 matched stars from wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020_astrometric_residuals.png (940 matched stars from wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021_astrometric_residuals.png (942 matched stars from wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits'
Saving fully-calibrated image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits'
Preparing the HTML report for the field Gem-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33130_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
Preparing report for the candidate 33130_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33131_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
Preparing report for the candidate 33131_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33132_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
Preparing report for the candidate 33132_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14622_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 14622_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:43:02.47 +23:26:56.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Gem-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
SExtractor catalog cache: saved Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Creating symlink local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits exists and is non-empty
wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits exists and is non-empty
wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits exists and is non-empty
wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits (1st reference image)
verification OK: wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Image size: 941.6'x627.1' 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: 07:22:55.118 +21:59:39.20 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-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits (1st new image)
verification OK: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Image size: 941.6'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:23:10.851 +21:59:34.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:22:55.118 +21:59:39.20
Second-epoch image center 07:23:10.851 +21:59:34.32
Angular distance between the image centers 0.0608 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits (2nd new image)
verification OK: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Image size: 941.6'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:23:13.966 +21:59:36.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:22:55.118 +21:59:39.20
Second-epoch image center 07:23:13.966 +21:59:36.20
Angular distance between the image centers 0.0728 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 07:23:10.851 +21:59:34.32
Second-epoch second image center 07:23:13.966 +21:59:36.20
Angular distance between the image centers 0.01205 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits &> /tmp/tmp.WcCfAOUwJY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.hG5p42KFUk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits &> /tmp/tmp.ZI8ycDoDnZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits &> /tmp/tmp.FSAzJaDXU5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits and wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits and wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
Found non-empty wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits and wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
The reference image (wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits) and catalog (wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat) found
'wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat' -> 'wcsmag.cat'
Read 153680 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 101.7461 to 119.3352 deg, Dec +16.3007 to +27.3487 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 101.7461 to 119.3352 deg, Dec 16.3007 to 27.3487 deg
Loaded 14554 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): 8811 out of 12036 total matches.
Matched with Tycho-2 12036 out of 153680 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.769600
a=0.000000 b=1.000000 c=22.769600
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 153680 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 101.7461 to 119.3352 deg, Dec +16.3007 to +27.3487 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 101.7461 to 119.3352 deg, Dec 16.3007 to 27.3487 deg
Loaded 14554 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): 8811 out of 12036 total matches.
Matched with Tycho-2 12036 out of 153680 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits:
Forced-photometry filter: calibrated wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits -> calib.txt_param_ref_wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits (aperture=4.7)
Read 151496 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 102.0337 to 119.6237 deg, Dec +16.4751 to +27.2973 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 102.0337 to 119.6237 deg, Dec 16.4751 to 27.2973 deg
Loaded 14001 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): 8799 out of 12010 total matches.
Matched with Tycho-2 12010 out of 151496 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits:
Forced-photometry filter: calibrated wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits -> calib.txt_param_ref_wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 28 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
2.1 pix Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
3.0 pix fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
3.0 pix fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
1.9 pix wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
2.1 pix wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
Limiting magnitude estimates:
15.4 mag. Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
15.4 mag. Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
13.6 mag. fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
13.6 mag. fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.WcCfAOUwJY (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.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-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits' -> 'wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=17863, passed=153629
Got 153629 stars (including 135492 good ones) from the SExtractor catalog wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 153629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 151026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 151027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 151027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits N_match=953 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.390 sigma_q3_arcsec=0.360 sigma_q4_arcsec=0.272 n_q1=232 n_q2=238 n_q3=246 n_q4=237 worst_quadrant_to_overall_ratio=1.100
The image catalog is written to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits -region wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hG5p42KFUk (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.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-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits' -> 'wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=17705, passed=151450
Got 151450 stars (including 133487 good ones) from the SExtractor catalog wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 151450 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 148360 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 148361 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 148362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 951 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits N_match=951 sigma_overall_arcsec=0.445 sigma_q1_arcsec=0.463 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.435 sigma_q4_arcsec=0.378 n_q1=182 n_q2=266 n_q3=224 n_q4=279 worst_quadrant_to_overall_ratio=1.058
The image catalog is written to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZI8ycDoDnZ (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1007, passed=30468
Got 30468 stars (including 29427 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 30468 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 29036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 29034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 29034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits N_match=941 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.557 sigma_q3_arcsec=0.445 sigma_q4_arcsec=0.487 n_q1=308 n_q2=223 n_q3=306 n_q4=104 worst_quadrant_to_overall_ratio=1.229
The image catalog is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits -region wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FSAzJaDXU5 (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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=936, passed=30243
Got 30243 stars (including 29275 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 30243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 28706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 28707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 28707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits N_match=942 sigma_overall_arcsec=0.479 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.561 sigma_q3_arcsec=0.475 sigma_q4_arcsec=0.495 n_q1=310 n_q2=221 n_q3=311 n_q4=100 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits -region wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits.cat.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-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-54-39_20.00sec_-0.00C_LIGHTs_0020.fits
Saving fully-calibrated image wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.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_2026-05-25_CI_Gem-04-Q1b1x1_215909_TTUQ1b1x1_793570_48Rzz4AT/wcs_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021.fits
Preparing the HTML report for the field Gem-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits at 07:11:27.19 +26:25:33.2: 12.53 +/- 0.02 detection
Forced photometry on wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits at 07:11:27.19 +26:25:33.2: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter REJECTED candidate at 07:11:27.19 +26:25:33.2: ref_mag=12.53 +/- 0.01 new_mean_mag=12.2136 delta=0.32 (need > 0.90)
Forced photometry on wcs_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits at 07:21:58.30 +26:27:31.8: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Gem-04-Q1b1x1_2026-02-21_22-26-53_20.00sec_-15.00C_LIGHT_0153.fits at 07:21:58.30 +26:27:31.8: 16.09 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out181696.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 181121_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
Preparing report for the candidate 181121_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
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Considering the candidate 181122_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
Preparing report for the candidate 181122_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
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Considering the candidate 181123_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
Preparing report for the candidate 181123_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
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Considering the candidate 181323_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181323_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:43:57.75 +25:46:40.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181338_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181338_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:46:15.08 +18:30:22.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181347_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181347_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:12:19.23 +24:07:16.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181419_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181419_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:43:14.52 +22:23:12.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181424_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181424_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181518_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181518_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:26:19.05 +25:55:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181525_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181525_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:26:25.39 +25:56:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181553_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181553_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:27:42.17 +22:10:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181567_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181567_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:21:48.53 +20:26:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181594_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181594_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:53:08.50 +20:10:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181607_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181607_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:32:08.80 +23:56:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181612_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181612_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:46:57.07 +26:00:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181641_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181641_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:17:42.49 +21:18:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181643_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181643_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:17:20.48 +26:22:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181644_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181644_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:38:21.47 +26:41:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181659_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181659_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:28:39.37 +26:48:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181664_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181664_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:42:53.28 +24:07:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181693_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181693_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:31:54.38 +24:32:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181696_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
Preparing report for the candidate 181696_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
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Considering the candidate 181699_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 181699_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:35:49.42 +24:54:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102023_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 102023_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:43:02.47 +23:26:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95880_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 95880_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:42:46.35 +23:09:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168691_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 168691_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:57:29.29 +26:03:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119081_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 119081_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 07:19:12.47 +26:47:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132602_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021
The candidate 132602_fd_Gem-04-Q1b1x1_2026-05-25_21-55-23_20.00sec_0.00C_LIGHTs_0021 did not pass the final checks
