This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,7.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 7.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,7.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 7.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,7.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 7.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.7123,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.2123 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7123,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2123 14.32CV 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: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
First image: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461143.71256128 13.04.2026 05:05:55.295 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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: 5 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): 15036
Objects passed selection criteria: 14979
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 12198.2
Average stars matched: 11937.8 (97.8644 %)
Memory usage VmPeak: 122288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:12:00 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: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
First image: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461143.71256128 13.04.2026 05:05:55.295 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 154
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 37 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): 103681
Objects passed selection criteria: 103454
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 86995.2
Average stars matched: 84124.5 (96.7001 %)
Memory usage VmPeak: 1945400 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:13:55 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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: 2461143.71199782
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
Saving wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits to local_wcs_cache/
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
Saving wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits to local_wcs_cache/
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits'
wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:22:41.275 +21:59:03.91
Angular distance between the image centers 0.0923 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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:22:40.440 +21:59:00.74
Angular distance between the image centers 0.0956 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 07:22:41.275 +21:59:03.91
Second-epoch second image center 07:22:40.440 +21:59:00.74
Angular distance between the image centers 0.00334 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits &> /tmp/tmp.A2cSiN1ytB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits &> /tmp/tmp.y8Hn1U7FiN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits &> /tmp/tmp.D743E0oM6W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits &> /tmp/tmp.EfH7DRyXBA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat' -> 'wcsmag.cat'
Read 24052 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 102.0354 to 119.5901 deg, Dec +16.4821 to +27.2938 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 102.0354 to 119.5901 deg, Dec 16.4821 to 27.2938 deg
Loaded 13967 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): 10770 out of 11768 total matches.
Matched with Tycho-2 11768 out of 24052 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914404
a=0.000000 b=1.000000 c=22.914404
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
2.2 pix Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
2.7 pix fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
2.7 pix fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Limiting magnitude estimates:
15.3 mag. Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
15.3 mag. Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
14.2 mag. fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
14.3 mag. fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.6 (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.A2cSiN1ytB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2144, passed=24052
Got 24052 stars (including 21876 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
util/solve_plate_with_UCAC5 got 24052 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 22930 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 22932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 22932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 947 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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.y8Hn1U7FiN (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2184, passed=23896
Got 23896 stars (including 21676 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 23896 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 22789 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 22792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 22792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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.D743E0oM6W (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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=723, passed=12091
Got 12091 stars (including 11358 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat
util/solve_plate_with_UCAC5 got 12091 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 11834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 11833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 11833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 937 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.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.EfH7DRyXBA (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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=687, passed=12265
Got 12265 stars (including 11566 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat
util/solve_plate_with_UCAC5 got 12265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 11988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 11987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 11987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
Saving fully-calibrated image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits'
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits'
Preparing the HTML report for the field Gem-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30892_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 30892_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:30.06 +22:51:27.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30900_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 30900_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:22.48 +22:47:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30996_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 30996_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:31:39.93 +25:31:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09360_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 09360_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:07:21.48 +22:42:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07610_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 07610_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:43:02.32 +23:26:56.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Gem-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Creating symlink local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits exists and is non-empty
wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:22:41.275 +21:59:03.91
Angular distance between the image centers 0.0923 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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:22:40.440 +21:59:00.74
Angular distance between the image centers 0.0956 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 07:22:41.275 +21:59:03.91
Second-epoch second image center 07:22:40.440 +21:59:00.74
Angular distance between the image centers 0.00334 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits &> /tmp/tmp.F4DYOKn5s0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits &> /tmp/tmp.oS98UNbtAB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits &> /tmp/tmp.zt9YYoDtOT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits &> /tmp/tmp.w3pWathehQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat' -> 'wcsmag.cat'
Read 150538 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 102.0340 to 119.6236 deg, Dec +16.4753 to +27.2952 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 102.0340 to 119.6236 deg, Dec 16.4753 to 27.2952 deg
Loaded 13999 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): 9026 out of 11981 total matches.
Matched with Tycho-2 11981 out of 150538 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774089
a=0.000000 b=1.000000 c=22.774089
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 104 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
2.0 pix Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
2.4 pix fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
2.4 pix fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Limiting magnitude estimates:
15.5 mag. Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
15.5 mag. Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
14.5 mag. fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
14.5 mag. fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (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.F4DYOKn5s0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=16511, passed=150509
Got 150509 stars (including 133763 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
util/solve_plate_with_UCAC5 got 150509 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 147846 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 147844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 147844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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.oS98UNbtAB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=16925, passed=153524
Got 153524 stars (including 136352 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 153524 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 149228 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 149228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 149227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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.zt9YYoDtOT (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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=5317, passed=78252
Got 78252 stars (including 72842 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat
util/solve_plate_with_UCAC5 got 78252 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 76636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 76639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 76639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.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.w3pWathehQ (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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=5204, passed=78044
Got 78044 stars (including 72755 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat
util/solve_plate_with_UCAC5 got 78044 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 76658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 76659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 76659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Saving fully-calibrated image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-06_20.00sec_-5.00C_LIGHT_0372.fits
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.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_2026-04-13_CI_Gem-04-Q2b1x1_000650_TTUQ2b1x1_14898_pX4ocU9q/wcs_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373.fits
Preparing the HTML report for the field Gem-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out170785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out171017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171786.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 6s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170782_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170782_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:14:32.90 +20:50:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170785_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170785_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:37:16.24 +25:08:56.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170787_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170787_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:19:05.80 +19:57:33.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170793_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170793_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:18:22.89 +17:52:04.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170794_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170794_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:20:42.06 +18:46:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170797_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170797_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:23:19.35 +20:37:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170800_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170800_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:48:24.03 +23:03:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.759 675329662506773760 117.09930214197 +23.06354711688 13.5026 12.9781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170803_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170803_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:31:11.32 +21:42:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.262 865230748146213120 112.79653008426 +21.71196205469 14.2222 13.8506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170810_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170810_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:38:10.76 +20:05:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.313 672631259110765568 114.54445141696 +20.08648222346 13.5426 13.1031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170818_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170818_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:12.08 +18:17:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.705 3361610742975907840 107.04984796098 +18.28819626726 13.5454 12.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170824_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170824_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:05:43.09 +19:37:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.488 3364959851095867264 106.42919513757 +19.62774627259 13.2744 12.5251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170825_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170825_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:13:49.39 +19:58:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170826_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170826_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:40:51.66 +19:08:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170837_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170837_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:05:41.81 +17:47:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.953 3361477461550769408 106.42447357908 +17.79574588260 13.4541 13.0463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170840_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170840_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:47:59.65 +18:49:09.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170841_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170841_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:06.09 +18:41:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.547 3361825972376511488 107.02492727157 +18.69915190696 13.1924 12.7686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170851_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170851_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:29.73 +19:50:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170852_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170852_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:05:00.11 +19:41:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.663 3365002495828550400 106.25026857562 +19.69465022989 12.4659 11.7955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170861_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 170861_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170862_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 170862_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170863_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 170863_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170889_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170889_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:22.48 +22:47:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170936_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170936_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170950_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170950_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170978_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 170978_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:21.05 +22:51:13.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171017_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 171017_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171018_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171018_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:01.57 +22:51:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171035_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171035_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:12:19.29 +24:07:15.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171045_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171045_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171047_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171047_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:56.05 +22:53:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171066_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171066_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:47.69 +22:50:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171069_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 171069_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171078_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171078_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:26:25.40 +25:56:20.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171084_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171084_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:04.72 +22:56:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171086_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171086_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171133_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171133_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:32:08.86 +23:56:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171134_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171134_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:12:35.78 +20:57:33.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171143_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171143_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:15.86 +22:50:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171171_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171171_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:00.69 +22:44:42.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171186_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171186_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:31:54.36 +24:32:03.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171193_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171193_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:04:06.49 +18:39:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171230_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171230_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:12:45.91 +25:33:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171233_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171233_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:44.07 +22:47:42.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171235_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171235_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:06:45.89 +23:15:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.918 3368456749046604928 106.69072311975 +23.25120853732 13.1957 12.8963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171258_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171258_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:44.00 +22:52:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171268_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171268_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:15.39 +21:47:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171273_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171273_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:07:22.53 +20:30:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171281_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171281_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171299_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171299_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:14:03.56 +19:28:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171305_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171305_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:26:55.50 +21:31:09.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171309_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171309_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171359_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171359_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171379_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171379_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:19:45.63 +20:26:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.852 3363744242210248320 109.93965485058 +20.44756748257 13.4697 13.0790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171389_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171389_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:06:11.18 +20:06:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171391_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171391_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:26:23.00 +18:10:09.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171406_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171406_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:28.30 +22:46:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171417_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171417_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:41:33.16 +18:14:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171426_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171426_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171428_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171428_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:47.24 +22:45:03.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171437_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171437_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:16:10.92 +24:39:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 3.366 870520468526028672 109.04637445328 +24.65128548348 13.2078 12.4772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171446_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171446_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:22:13.65 +22:40:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171449_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171449_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:27:03.72 +20:16:02.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171467_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171467_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:27:24.67 +19:09:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171473_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171473_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:03:52.42 +20:07:18.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171480_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171480_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:05:47.37 +18:57:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171481_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 171481_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171498_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171498_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:30:28.14 +25:27:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171503_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171503_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:25:02.84 +19:56:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.151 3362951597405009792 111.26099506535 +19.94277011616 13.5857 13.1393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171506_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171506_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:10:01.72 +21:27:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171507_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171507_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:12:20.17 +24:08:07.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171511_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171511_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:07:26.82 +19:37:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171513_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171513_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:16:17.10 +22:39:54.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171515_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171515_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:13:43.21 +26:00:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171523_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171523_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:10:22.73 +20:00:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171526_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171526_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:09.83 +22:42:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171527_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171527_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:15:40.95 +22:08:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.549 3367254604879504640 108.92120419048 +22.14817293916 13.9804 13.5305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171542_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 171542_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171545_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171545_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:35:19.15 +18:19:11.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171557_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171557_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:38.96 +22:44:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171565_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171565_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:12:40.76 +21:21:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171572_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171572_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171579_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171579_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:38:41.86 +20:52:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.929 673114803708370304 114.67397776914 +20.87492507729 13.8325 13.1684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171580_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171580_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:29:33.84 +23:02:48.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171586_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171586_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:24:29.49 +18:53:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171593_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171593_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:41.53 +22:45:27.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171596_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 171596_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171619_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171619_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:09.08 +22:50:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171628_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171628_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:42.67 +20:49:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171633_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171633_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:14.38 +19:32:12.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171653_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171653_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:24:12.12 +21:26:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171654_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171654_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:30:20.02 +20:47:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.888 864926183426832896 112.58336876388 +20.78603519374 14.2637 13.7339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171659_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171659_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:22.40 +21:13:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171672_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 171672_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171680_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171680_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:11:39.95 +20:41:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171683_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171683_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:20:22.85 +19:59:40.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171684_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171684_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:09:07.62 +22:49:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171691_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171691_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:14:39.43 +25:20:31.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171745_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171745_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:20:43.88 +22:50:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.141 869259259968095488 110.18193896591 +22.84118581699 14.7583 14.2962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171746_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171746_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:20:30.14 +22:26:09.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171759_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171759_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171760_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 171760_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:08:39.45 +22:48:48.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171786_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
Preparing report for the candidate 171786_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47884_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 47884_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
**** FOUND 07:43:02.31 +23:26:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61021_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373
The candidate 61021_fd_Gem-04-Q2b1x1_2026-04-13_00-05-55_20.00sec_-4.90C_LIGHT_0373 did not pass the final checks
