This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 03.4554 2461255.9554 9.91 07:07:54.98 +29:40:47.2
187.49168 16.33954 galactic Gem Second-epoch detections are separated by 1.9" and 8.9 pix
The object was found in VSX 1" ASASSN-V J070755.05+294047.7
Type: SR
# Max. Min./Amp. JD0 Period
11.830 g Y 0.850 g 2459118.04000 726.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 07:07:54.98 +29:40:47.2: 10.87 +/- 0.00 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 07:07:54.98 +29:40:47.2: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
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
ASASSN-V J070755.05+294047.7,2461255.9554,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070755.05+294047.7 20260803.4554 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4554 2461255.9554 9.70 07:14:45.13 +34:06:30.7
183.71163 19.30102 galactic Gem Second-epoch detections are separated by 0.9" and 8.3 pix
The object was found in VSX 2" [D2006] LCG10
Type: L
# Max. Min./Amp. JD0 Period
11.370 V Y 0.390 w
The object was not found in astcheck.
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 07:14:45.13 +34:06:30.7: 10.76 +/- 0.00 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 07:14:45.13 +34:06:30.7: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
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
[D2006] LCG10,2461255.9554,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
[D2006] LCG10 20260803.4554 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4554 2461255.9554 10.17 07:16:33.93 +25:59:44.5
191.80440 16.70173 galactic Gem Second-epoch detections are separated by 0.7" and 9.2 pix
The object was found in VSX 2" WZ Gem
Type: M
# Max. Min./Amp. JD0 Period
9.000 V 16.300 V 2453720.00000 333.000000000000 M3e
The object was not found in astcheck.
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 07:16:33.93 +25:59:44.5: 11.82 +/- 0.01 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 07:16:33.93 +25:59:44.5: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
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
WZ Gem,2461255.9554,10.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WZ Gem 20260803.4554 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4554 2461255.9554 12.59 06:36:14.13 +29:06:14.0
185.15061 9.80201 galactic Aur Second-epoch detections are separated by 1.6" and 9.3 pix
The object was found in VSX 1" ASASSN-V J063614.18+290615.0
Type: EA
# Max. Min./Amp. JD0 Period
12.640 V 13.830 V 2457370.00900 1.479600000000
The object was not found in astcheck.
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 06:36:14.13 +29:06:14.0: 13.66 +/- 0.04 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 06:36:14.13 +29:06:14.0: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
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
ASASSN-V J063614.18+290615.0,2461255.9554,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063614.18+290615.0 20260803.4554 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
First image: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Last image: 2461255.95579617 03.08.2026 10:56:10.789 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.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.: -7.57
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 18332
Objects passed selection criteria: 18190
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 11170
Average stars matched: 10864.5 (97.265 %)
Memory usage VmPeak: 244728 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 06:35:36 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: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
First image: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Last image: 2461255.95579617 03.08.2026 10:56:10.789 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 30
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 19 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 130765
Objects passed selection criteria: 130353
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: 86000.2
Average stars matched: 82687.2 (96.1477 %)
Memory usage VmPeak: 604772 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 06:36:37 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.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: 2461255.95498394
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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits'
wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits'
wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits exists and is non-empty
Saving wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits to local_wcs_cache/
'wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits' -> 'local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits'
wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits exists and is non-empty
Saving wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits to local_wcs_cache/
'wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits' -> 'local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:00:00.338 +29:59:43.36 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-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits (1st new image)
verification OK: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Image size: 941.1'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 07:00:14.041 +29:58:26.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:00:00.338 +29:59:43.36
Second-epoch image center 07:00:14.041 +29:58:26.07
Angular distance between the image centers 0.0539 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits (2nd new image)
verification OK: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 07:00:11.828 +29:59:08.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:00:00.338 +29:59:43.36
Second-epoch image center 07:00:11.828 +29:59:08.88
Angular distance between the image centers 0.0426 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 07:00:14.041 +29:58:26.07
Second-epoch second image center 07:00:11.828 +29:59:08.88
Angular distance between the image centers 0.01432 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits &> /tmp/tmp.eTxoV79LLd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.eFnlFNATXg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits &> /tmp/tmp.T8c7MINGw2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits &> /tmp/tmp.Lc4GNKkWSD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
The reference image (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits) and catalog (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat) found
'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat' -> 'wcsmag.cat'
Read 24243 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2299 to 114.2898 deg, Dec +24.1612 to +35.3654 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 95.2299 to 114.2898 deg, Dec 24.1612 to 35.3654 deg
Loaded 15250 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): 10848 out of 11975 total matches.
Matched with Tycho-2 11975 out of 24243 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.903450
a=0.000000 b=1.000000 c=22.903450
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24243 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2299 to 114.2898 deg, Dec +24.1612 to +35.3654 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 95.2299 to 114.2898 deg, Dec 24.1612 to 35.3654 deg
Loaded 15250 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): 10848 out of 11975 total matches.
Matched with Tycho-2 11975 out of 24243 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Forced-photometry filter: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits (aperture=6.1)
Read 24037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2298 to 114.2895 deg, Dec +24.1920 to +35.3691 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 95.2298 to 114.2895 deg, Dec 24.1920 to 35.3691 deg
Loaded 15195 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): 10824 out of 11955 total matches.
Matched with Tycho-2 11955 out of 24037 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Forced-photometry filter: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits (aperture=6.1)
____ 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: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
2.1 pix Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
2.2 pix fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
2.3 pix fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Limiting magnitude estimates:
15.3 mag. Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
15.3 mag. Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
12.8 mag. fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
12.8 mag. fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.eTxoV79LLd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2293, bad_region=4438, passed=24243
Got 24243 stars (including 17882 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 24243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 4829 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 4769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 20793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 20793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 20793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4768 stars left (next iteration limit 5245)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits N_match=4768 sigma_overall_arcsec=0.404 sigma_q1_arcsec=0.482 sigma_q2_arcsec=0.344 sigma_q3_arcsec=0.341 sigma_q4_arcsec=0.296 n_q1=1752 n_q2=820 n_q3=1429 n_q4=767 worst_quadrant_to_overall_ratio=1.195
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eFnlFNATXg (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2282, bad_region=4407, passed=24037
Got 24037 stars (including 17688 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 24037 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 4826 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 4768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4766 matched stars entering correct_measured_positions(), 20608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 4827 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 20608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 20608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4768 stars left (next iteration limit 5242)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits N_match=4768 sigma_overall_arcsec=0.394 sigma_q1_arcsec=0.457 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.299 n_q1=1744 n_q2=821 n_q3=1437 n_q4=766 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.T8c7MINGw2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=325, bad_region=430, passed=3263
Got 3263 stars (including 2530 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat
util/solve_plate_with_UCAC5 got 3263 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 2450 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2415 matched stars entering correct_measured_positions(), 2417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2414 matched stars entering correct_measured_positions(), 2923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 2450 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2412 matched stars entering correct_measured_positions(), 2923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 2412 matched stars entering correct_measured_positions(), 2923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 2412 stars left (next iteration limit 2655)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2412 robust_rms=5.597 arcsec worst_quadrant_rms=13.083 arcsec
SIP_REFIT: SIP order 3 trial: matched=2412 robust_rms=0.589 arcsec worst_quadrant_rms=0.606 arcsec
SIP_REFIT: SIP order 5 trial: matched=2412 robust_rms=0.537 arcsec worst_quadrant_rms=0.547 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2412 robust_rms_before=1.514 arcsec robust_rms_before_corrected=0.603 arcsec robust_rms_after=0.537 arcsec worst_quadrant_rms_before=0.689 worst_quadrant_rms_after=0.547
verification OK: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
verification OK: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Image size: 941.7'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 07:00:14.151 +29:58:24.48 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3263 stars ###
'wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/correct_sextractor_wcs_catalog_usingxy2sky2592391.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.514 -> 0.537 arcsec)
WCS_QUALITY_DIAG: file=fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits N_match=2412 sigma_overall_arcsec=0.574 sigma_q1_arcsec=0.633 sigma_q2_arcsec=0.568 sigma_q3_arcsec=0.583 sigma_q4_arcsec=0.539 n_q1=971 n_q2=339 n_q3=787 n_q4=315 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits -region wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Lc4GNKkWSD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=343, bad_region=418, passed=3160
Got 3160 stars (including 2427 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat
util/solve_plate_with_UCAC5 got 3160 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 2347 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2318 matched stars entering correct_measured_positions(), 2320 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2318 matched stars entering correct_measured_positions(), 2818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 2350 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2318 matched stars entering correct_measured_positions(), 2818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 2318 matched stars entering correct_measured_positions(), 2818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 2318 stars left (next iteration limit 2549)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2318 robust_rms=5.683 arcsec worst_quadrant_rms=13.416 arcsec
SIP_REFIT: SIP order 3 trial: matched=2318 robust_rms=0.659 arcsec worst_quadrant_rms=0.759 arcsec
SIP_REFIT: SIP order 5 trial: matched=2318 robust_rms=0.555 arcsec worst_quadrant_rms=0.642 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2318 robust_rms_before=1.435 arcsec robust_rms_before_corrected=0.593 arcsec robust_rms_after=0.555 arcsec worst_quadrant_rms_before=0.698 worst_quadrant_rms_after=0.642
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.698 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits N_match=2318 sigma_overall_arcsec=0.582 sigma_q1_arcsec=0.653 sigma_q2_arcsec=0.550 sigma_q3_arcsec=0.531 sigma_q4_arcsec=0.552 n_q1=945 n_q2=328 n_q3=747 n_q4=298 worst_quadrant_to_overall_ratio=1.122
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits -region wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits sigma_overall=0.404 worst_q_ratio=1.195
ref2=Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits sigma_overall=0.394 worst_q_ratio=1.161
new1=fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits sigma_overall=0.574 worst_q_ratio=1.102
new2=fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits sigma_overall=0.582 worst_q_ratio=1.122
reference average sigma_overall=0.399 worst_q_ratio=1.178
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226_astrometric_residuals.png (4768 matched stars from wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227_astrometric_residuals.png (4768 matched stars from wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518_astrometric_residuals.png (2412 matched stars from wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519_astrometric_residuals.png (2318 matched stars from wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits'
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits'
Preparing the HTML report for the field Gem-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 07:07:54.98 +29:40:47.2: 10.87 +/- 0.00 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 07:14:45.13 +34:06:30.7: 10.76 +/- 0.00 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 07:16:33.93 +25:59:44.5: 11.82 +/- 0.01 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 07:14:45.13 +34:06:30.7: 10.76 +/- 0.00 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 07:07:54.98 +29:40:47.2: 10.87 +/- 0.00 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 07:16:33.93 +25:59:44.5: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter KEPT candidate at 07:14:45.13 +34:06:30.7: ref_mag=10.76 +/- 0.00 new_mean_mag=9.6980 delta=1.06 (need > 0.90)
Forced photometry filter KEPT candidate at 07:07:54.98 +29:40:47.2: ref_mag=10.87 +/- 0.00 new_mean_mag=9.9171 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 07:16:33.93 +25:59:44.5: ref_mag=11.81 +/- 0.01 new_mean_mag=10.1722 delta=1.63 (need > 0.90)
Adding exclusion_list_local.txt__out03075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21515.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11996_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
Preparing report for the candidate 11996_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21515_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
Preparing report for the candidate 21515_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03075_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
Preparing report for the candidate 03075_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13804_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 13804_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:47:07.28 +30:16:34.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Gem-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:16:33.93 +25:59:44.5
07:07:54.98 +29:40:47.2
07:14:45.13 +34:06:30.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits exists and is non-empty
wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits exists and is non-empty
wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:00:00.338 +29:59:43.36 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-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits (1st new image)
verification OK: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Image size: 941.1'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 07:00:14.041 +29:58:26.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:00:00.338 +29:59:43.36
Second-epoch image center 07:00:14.041 +29:58:26.07
Angular distance between the image centers 0.0539 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits (2nd new image)
verification OK: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 07:00:11.828 +29:59:08.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:00:00.338 +29:59:43.36
Second-epoch image center 07:00:11.828 +29:59:08.88
Angular distance between the image centers 0.0426 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 07:00:14.041 +29:58:26.07
Second-epoch second image center 07:00:11.828 +29:59:08.88
Angular distance between the image centers 0.01432 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits &> /tmp/tmp.DcGwyjRA9E
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.NvxbTmso6n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits &> /tmp/tmp.67ZvXovJVz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits &> /tmp/tmp.IDFYYWjXtU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
The reference image (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits) and catalog (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat) found
'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat' -> 'wcsmag.cat'
Read 167542 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.1852 to 114.3067 deg, Dec +24.1432 to +35.3660 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 95.1852 to 114.3067 deg, Dec 24.1432 to 35.3660 deg
Loaded 15347 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): 8758 out of 12241 total matches.
Matched with Tycho-2 12241 out of 167542 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.764400
a=0.000000 b=1.000000 c=22.764400
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167542 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.1852 to 114.3067 deg, Dec +24.1432 to +35.3660 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 95.1852 to 114.3067 deg, Dec 24.1432 to 35.3660 deg
Loaded 15347 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): 8758 out of 12241 total matches.
Matched with Tycho-2 12241 out of 167542 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Forced-photometry filter: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits (aperture=4.6)
Read 166985 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2096 to 114.3128 deg, Dec +24.1626 to +35.3760 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 95.2096 to 114.3128 deg, Dec 24.1626 to 35.3760 deg
Loaded 15290 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): 8659 out of 12225 total matches.
Matched with Tycho-2 12225 out of 166985 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Forced-photometry filter: calibrated wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
1.9 pix Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
2.1 pix fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
2.1 pix fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Limiting magnitude estimates:
15.5 mag. Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
15.5 mag. Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
13.3 mag. fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
13.2 mag. fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DcGwyjRA9E (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=20873, bad_region=23130, passed=167504
Got 167504 stars (including 125190 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 167504 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 4808 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 4773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 149932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 4809 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 149932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 149932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4772 stars left (next iteration limit 5250)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits N_match=4772 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.446 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.276 n_q1=1652 n_q2=856 n_q3=1476 n_q4=788 worst_quadrant_to_overall_ratio=1.233
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NvxbTmso6n (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=20907, bad_region=23158, passed=166940
Got 166940 stars (including 124617 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 166940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 4801 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4762 matched stars entering correct_measured_positions(), 4763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4762 matched stars entering correct_measured_positions(), 149289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 4801 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 149289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4763 matched stars entering correct_measured_positions(), 149289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4763 stars left (next iteration limit 5238)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits N_match=4763 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.445 sigma_q2_arcsec=0.344 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.289 n_q1=1663 n_q2=845 n_q3=1465 n_q4=790 worst_quadrant_to_overall_ratio=1.256
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.67ZvXovJVz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1195, bad_region=2115, passed=31778
Got 31778 stars (including 28508 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat
util/solve_plate_with_UCAC5 got 31778 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4752 matched stars entering correct_measured_positions(), 4756 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4752 matched stars entering correct_measured_positions(), 30268 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4753 matched stars entering correct_measured_positions(), 30268 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4753 matched stars entering correct_measured_positions(), 30268 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4753 stars left (next iteration limit 5227)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits N_match=4753 sigma_overall_arcsec=0.571 sigma_q1_arcsec=0.631 sigma_q2_arcsec=0.528 sigma_q3_arcsec=0.561 sigma_q4_arcsec=0.508 n_q1=1884 n_q2=575 n_q3=1598 n_q4=696 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits -region wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IDFYYWjXtU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1025, bad_region=1992, passed=30095
Got 30095 stars (including 27104 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat
util/solve_plate_with_UCAC5 got 30095 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4824 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4750 matched stars entering correct_measured_positions(), 4753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4750 matched stars entering correct_measured_positions(), 28689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4824 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4753 matched stars entering correct_measured_positions(), 28689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4753 matched stars entering correct_measured_positions(), 28689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4753 stars left (next iteration limit 5225)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits N_match=4753 sigma_overall_arcsec=0.566 sigma_q1_arcsec=0.624 sigma_q2_arcsec=0.523 sigma_q3_arcsec=0.533 sigma_q4_arcsec=0.534 n_q1=1876 n_q2=574 n_q3=1612 n_q4=691 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits -region wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-55-00_20.00sec_0.00C_LIGHT_0518.fits
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Gem-01-Q2b1x1_063239_TTUQ2b1x1_2584373_SCVu0l10/wcs_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519.fits
Preparing the HTML report for the field Gem-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 06:50:38.72 +26:04:25.0: 11.98 +/- 0.01 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 06:40:04.10 +31:41:49.6: 12.99 +/- 0.02 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 06:40:04.10 +31:41:49.6: 12.91 +/- 0.02 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 06:50:38.72 +26:04:25.0: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter REJECTED candidate at 06:40:04.10 +31:41:49.6: ref_mag=12.95 +/- 0.01 new_mean_mag=12.9495 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:50:38.72 +26:04:25.0: ref_mag=11.98 +/- 0.01 new_mean_mag=12.2269 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits at 06:36:14.13 +29:06:14.0: 13.66 +/- 0.04 detection
Forced photometry on wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits at 06:36:14.13 +29:06:14.0: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 06:36:14.13 +29:06:14.0: ref_mag=13.65 +/- 0.03 new_mean_mag=12.5488 delta=1.11 (need > 0.90)
Adding exclusion_list_local.txt__out80230.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 190143_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190143_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
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Considering the candidate 190147_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190147_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:43:19.24 +26:58:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190151_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190151_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
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Considering the candidate 190163_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190163_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:53:43.91 +29:29:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190164_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190164_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:47:04.51 +26:33:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190165_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190165_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:50:21.98 +29:19:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190229_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190229_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:52:42.40 +33:55:49.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 190232_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190232_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:57:06.64 +33:41:29.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190266_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190266_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:41:18.78 +29:41:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190268_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190268_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:35:16.87 +28:00:05.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190327_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190327_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:39:34.04 +28:18:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190328_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190328_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:35:05.43 +27:59:59.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190358_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190358_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:45:39.18 +27:38:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190361_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190361_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:54:05.49 +32:29:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190364_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190364_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:42:45.14 +32:52:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190454_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 190454_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 07:00:11.03 +29:44:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80230_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
Preparing report for the candidate 80230_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
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Considering the candidate 179521_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 179521_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:56:15.93 +29:41:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146225_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 146225_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:33:17.87 +31:35:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20138_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 20138_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 07:16:33.90 +25:59:45.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 96257_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 96257_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 06:47:07.23 +30:16:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84162_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 84162_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks
**** FOUND 07:07:54.96 +29:40:48.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 166693_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519
The candidate 166693_fd_Gem-01-Q2b1x1_2026-08-03_05-56-10_20.00sec_0.00C_LIGHT_0519 did not pass the final checks