This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DK Gem,2461136.7537,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DK Gem 20260406.2537 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7537,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2537 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7537,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2537 14.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 882217893558817920,2461136.7537,14.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 882217893558817920 20260406.2537 14.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7537,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2537 14.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7537,14.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2537 14.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AT Cnc,2461136.7537,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AT Cnc 20260406.2537 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.71692514 12.02.2026 05:12:12.332 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
First image: 2461083.71692514 12.02.2026 05:12:12.332 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Last image: 2461136.75410784 06.04.2026 06:05:44.917 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.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.: -7.50
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 14086
Objects passed selection criteria: 14056
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 11948.5
Average stars matched: 11628.2 (97.3197 %)
Memory usage VmPeak: 118608 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 01:07:45 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: 2461083.71692514 12.02.2026 05:12:12.332 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
First image: 2461083.71692514 12.02.2026 05:12:12.332 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Last image: 2461136.75410784 06.04.2026 06:05:44.917 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 70
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 42 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 88364
Objects passed selection criteria: 88141
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 77461
Average stars matched: 74721 (96.4627 %)
Memory usage VmPeak: 1876824 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 01:09:15 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
SExtractor catalog cache: saved Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat to cache
SExtractor catalog cache: saved Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.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: 2461136.75327076
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-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
Saving wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits to local_wcs_cache/
'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits' -> 'local_wcs_cache/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits'
wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
Saving wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits to local_wcs_cache/
'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits'
wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits exists and is non-empty
Saving wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits to local_wcs_cache/
'wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits' -> 'local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits'
wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits exists and is non-empty
Saving wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits to local_wcs_cache/
'wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits' -> 'local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:59:59.909 +29:59:55.65
Second-epoch image center 07:59:51.677 +29:59:23.48
Angular distance between the image centers 0.0310 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:59:59.909 +29:59:55.65
Second-epoch image center 07:59:50.736 +29:58:54.07
Angular distance between the image centers 0.0373 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 07:59:51.677 +29:59:23.48
Second-epoch second image center 07:59:50.736 +29:58:54.07
Angular distance between the image centers 0.00885 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.f0uv8BPAvD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.n9OU28WKXc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits &> /tmp/tmp.hzolZlAJp3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits &> /tmp/tmp.MB5orzHF8q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
Found non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
The reference image (wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits) and catalog (wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat) found
'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat' -> 'wcsmag.cat'
Read 14371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 110.1895 to 129.2995 deg, Dec +24.1558 to +35.3509 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 110.1895 to 129.2995 deg, Dec 24.1558 to 35.3509 deg
Loaded 9871 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): 7216 out of 7782 total matches.
Matched with Tycho-2 7782 out of 14371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.912020
a=0.000000 b=1.000000 c=22.912020
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
1.9 pix Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
2.2 pix fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
2.2 pix fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Limiting magnitude estimates:
15.4 mag. Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
15.4 mag. Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
14.8 mag. fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
14.8 mag. fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.f0uv8BPAvD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits' -> 'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1108, passed=14371
Got 14371 stars (including 13247 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 14371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 14189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14187 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14175 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 974 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.n9OU28WKXc (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1133, passed=14315
Got 14315 stars (including 13161 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 14315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 14143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14142 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hzolZlAJp3 (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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=688, passed=9696
Got 9696 stars (including 8995 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat
util/solve_plate_with_UCAC5 got 9696 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 9599 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
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 9600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 9600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits -region wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MB5orzHF8q (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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=694, passed=9677
Got 9677 stars (including 8973 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat
util/solve_plate_with_UCAC5 got 9677 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 9593 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
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 9592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 9592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits -region wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits'
Saving fully-calibrated image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits'
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits'
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits'
Preparing the HTML report for the field Gem-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out06746.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 20694_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 20694_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20695_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 20695_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:31:22.38 +30:08:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21217_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 21217_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:57:34.39 +26:51:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.130 874385281959736192 119.39327158847 +26.86419793797 12.2502 11.6179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12811_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 12811_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:26:13.97 +33:22:17.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06746_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
Preparing report for the candidate 06746_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Gem-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:31:11.04 +29:09:43.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
SExtractor catalog cache: saved Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat to cache
SExtractor catalog cache: saved Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Creating symlink local_wcs_cache/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits exists and is non-empty
wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:59:59.909 +29:59:55.65
Second-epoch image center 07:59:51.677 +29:59:23.48
Angular distance between the image centers 0.0310 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:59:59.909 +29:59:55.65
Second-epoch image center 07:59:50.736 +29:58:54.07
Angular distance between the image centers 0.0373 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 07:59:51.677 +29:59:23.48
Second-epoch second image center 07:59:50.736 +29:58:54.07
Angular distance between the image centers 0.00885 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.T3KMQ5m2zQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.qI3wuw48cN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits &> /tmp/tmp.MdRti80uX2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits &> /tmp/tmp.p7GeWgqLNY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
Found non-empty wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
The reference image (wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits) and catalog (wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat) found
'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat' -> 'wcsmag.cat'
Read 92293 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 110.1895 to 129.3003 deg, Dec +24.1558 to +35.3693 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 110.1895 to 129.3003 deg, Dec 24.1558 to 35.3693 deg
Loaded 9883 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): 6521 out of 7921 total matches.
Matched with Tycho-2 7921 out of 92293 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.781221
a=0.000000 b=1.000000 c=22.781221
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 67 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
1.8 pix Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
2.0 pix fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
2.1 pix fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Limiting magnitude estimates:
15.6 mag. Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
15.6 mag. Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
15.0 mag. fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
15.0 mag. fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.T3KMQ5m2zQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits' -> 'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=6631, passed=92272
Got 92272 stars (including 85483 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 92272 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 91201 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
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 91202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 91202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qI3wuw48cN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=6656, passed=92132
Got 92132 stars (including 85329 good ones) from the SExtractor catalog wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 92132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 91266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 91266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 91266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MdRti80uX2 (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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2886, passed=63890
Got 63890 stars (including 60894 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat
util/solve_plate_with_UCAC5 got 63890 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 63196 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
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 63196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 63196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits -region wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.p7GeWgqLNY (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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
WCS_IMAGE_NAME=wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
WCS-calibrated image found: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Checking if the catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat corresponding to the image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
WCS catalog name: wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2905, passed=63345
Got 63345 stars (including 60336 good ones) from the SExtractor catalog wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat
util/solve_plate_with_UCAC5 got 63345 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 62702 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
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 62702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 62702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits -region wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-12_20.00sec_-14.90C_LIGHT_0201.fits
Saving fully-calibrated image wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_Gem-02-Q1b1x1_2026-02-11_23-12-52_20.00sec_-15.00C_LIGHT_0202.fits
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-04-32_20.00sec_-4.90C_LIGHTs_0114.fits
Saving fully-calibrated image wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.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_2026-04-06_CI_Gem-02-Q1b1x1_010645_TTUQ1b1x1_26107_KOH9X1Yp/wcs_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115.fits
Preparing the HTML report for the field Gem-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out109305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out110295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112611.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 109305_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109305_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:10:28.76 +29:56:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.708 876744013574832640 122.61954057121 +29.93893075560 15.0070 14.4051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109310_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109310_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:36:39.30 +32:46:54.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)
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Considering the candidate 109312_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109312_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:14:44.34 +32:43:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109314_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109314_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:29:03.67 +32:47:29.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)
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Considering the candidate 109317_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109317_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:31:27.99 +29:33:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.486 707751962604178944 127.86653323127 +29.56294212705 14.1075 13.5541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109323_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109323_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:10:47.04 +34:02:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.820 902762788015514880 122.69604991394 +34.03519263026 13.7466 13.2460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109330_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109330_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 109530_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109530_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:01:58.07 +34:06:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 1.523 905546648377001984 120.49179977544 +34.10623682694 11.2918 10.9272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109538_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109538_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:34:52.07 +31:52:34.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 109792_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109792_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:52:23.77 +27:43:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.401 875415116334324992 118.09915975907 +27.72121131259 11.9516 11.5228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109925_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 109925_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:31:37.09 +32:14:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.692 892199848526876544 112.90502327809 +32.24093223212 12.4761 11.8777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110202_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110202_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:34:48.81 +31:51:46.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 110279_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110279_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:06:44.08 +32:01:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.570 877919322785449344 121.68384355824 +32.02833800648 13.1020 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110295_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
Preparing report for the candidate 110295_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
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Considering the candidate 110309_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110309_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:42:50.74 +34:00:37.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 110368_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110368_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:43:30.01 +35:02:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.232 894438179323517312 115.87534624707 +35.04637676679 12.9719 12.4474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110554_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110554_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:49:54.69 +27:26:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.356 875073851115994880 117.47827641148 +27.43412802438 13.2784 12.8698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110574_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110574_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:00:22.35 +25:02:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110605_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110605_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:46:19.01 +30:48:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110633_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110633_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:19:59.50 +27:14:39.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 110679_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110679_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:29:32.63 +32:29:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110743_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110743_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:51:20.13 +32:28:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.311 881005033449208320 117.83402353739 +32.47026930519 13.4277 12.7679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110801_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110801_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:31:33.29 +30:37:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.969 708131706432222080 127.88863072325 +30.62512388424 13.4471 12.9426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110932_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 110932_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:31:17.63 +29:14:21.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
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Considering the candidate 111039_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111039_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:23:01.95 +29:13:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.136 708235747720148608 125.75808488969 +29.22590243025 13.7266 13.2752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111071_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111071_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:58:05.96 +33:23:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.809 881472291531111936 119.52496436200 +33.38670408356 13.7759 13.4100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111074_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111074_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:31:23.44 +25:40:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.048 871658119461592320 112.84757195310 +25.67563939697 13.7708 13.2572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111084_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111084_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:03:06.80 +27:56:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.291 876032870070594304 120.77840844896 +27.94626843400 13.3762 12.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111096_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111096_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:13:15.68 +29:33:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111230_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111230_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:32:53.00 +31:03:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.864 708168574431389568 128.22062199089 +31.06544760153 13.9411 13.5462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111237_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111237_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:20:47.76 +26:57:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.294 682978556880724864 125.19928832451 +26.96030427386 13.8075 13.3456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111241_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111241_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:42:47.01 +32:00:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.727 880355630097971712 115.69567342106 +32.00125382857 14.0089 13.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111250_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111250_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:40:22.69 +28:48:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 5.527 878548140358273920 115.09453892763 +28.80688132670 14.0342 13.3797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111251_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111251_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:53:34.68 +30:36:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.749 880508707029783424 118.39462652269 +30.61237181262 14.0856 13.6316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111286_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111286_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:35:11.17 +31:36:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.075 709707993789969664 128.79689240136 +31.61019350890 14.0104 13.5877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111300_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111300_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:32:47.19 +28:58:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.959 873402185421219968 113.19659844043 +28.97379004769 13.5517 12.8179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111305_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111305_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:32:29.60 +30:45:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111331_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111331_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:56:43.51 +26:07:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111334_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111334_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:33:33.72 +30:50:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111404_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111404_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:41:21.77 +32:04:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.965 880371336794428288 115.34029704852 +32.07130209286 14.1438 13.7067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111454_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111454_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:16:36.34 +29:15:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.284 684449256762352896 124.15182468557 +29.26275551241 14.1374 13.6529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111476_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111476_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:33:02.20 +31:46:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111527_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111527_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:53:10.62 +32:11:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 2.608 880936588850528512 118.29379756677 +32.18457947123 14.1471 13.6594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111548_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111548_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:05:30.43 +32:29:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.406 902151356471719424 121.37687714618 +32.49628295457 13.9168 13.3260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111556_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111556_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:34:29.22 +25:13:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.013 868574882698850048 113.62180589039 +25.23058421289 14.1899 13.5280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111560_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111560_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:14:33.29 +25:57:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111634_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111634_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:37:00.69 +25:44:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111640_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111640_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:05:31.22 +26:08:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.679 681973843771007232 121.38026969930 +26.14147626689 13.9627 13.2856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111683_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111683_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:33:07.85 +31:29:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111768_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111768_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:55:58.54 +32:57:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 2.938 881359660309015808 118.99453196428 +32.95739554946 14.1997 13.6950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111774_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111774_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:09:51.54 +33:09:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.379 902282095275942144 122.46487218855 +33.15864218627 14.4996 13.8963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111778_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
Preparing report for the candidate 111778_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
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Considering the candidate 111894_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111894_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:39:29.98 +27:51:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 4.315 878278863087825280 114.87386813929 +27.85695443938 14.1546 13.7034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111911_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 111911_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:22:38.28 +30:44:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 2.082 708664179297666304 125.65938340574 +30.73515269553 14.4391 13.9158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112165_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 112165_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:48:29.69 +35:07:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.201 894592557627817984 117.12407057028 +35.13090209223 14.3192 13.6308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112179_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 112179_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:01:05.57 +31:43:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.634 878040406504009600 120.27373214316 +31.72946922470 14.6118 14.1563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112403_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
Preparing report for the candidate 112403_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
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Considering the candidate 112472_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 112472_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:56:54.44 +33:54:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.398 881568052121830144 119.22670610108 +33.90129667410 14.7019 14.1931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112519_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
Preparing report for the candidate 112519_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
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Considering the candidate 112544_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 112544_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:01:23.38 +25:49:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.58, MAG_FAINT_SEARCH_LIMIT=15.56)GAIADR2_OUTPUT=# 1.108 682044281235121024 120.34710240742 +25.82168448429 14.4841 13.9719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112592_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 112592_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:42:08.72 +34:39:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112611_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
Preparing report for the candidate 112611_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
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Considering the candidate 112630_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 112630_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:43:21.68 +35:02:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 1.283 894438213683160320 115.84076652980 +35.04410353406 14.5815 14.1396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112638_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 112638_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 08:06:13.48 +31:49:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.423 877907228157562368 121.55628681625 +31.81916910843 14.9909 14.4570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 69850_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 69850_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
**** FOUND 07:26:14.00 +33:22:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44359_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115
The candidate 44359_fd_Gem-02-Q1b1x1_2026-04-06_01-05-44_20.00sec_-5.00C_LIGHTs_0115 did not pass the final checks
