This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 594918047840470528,2461136.7403,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 594918047840470528 20260406.2403 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7403,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2403 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7403,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2403 13.74CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7403,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2403 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7403,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2403 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7403,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2403 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J135.0693+03.1792,2461136.7403,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J135.0693+03.1792 20260406.2403 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7403,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2403 12.97CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3078956711840391936,2461136.7403,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3078956711840391936 20260406.2403 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7403,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2403 13.12CV 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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461136.74061653 06.04.2026 05:46:19.268 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15053
Objects passed selection criteria: 15005
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 11713.5
Average stars matched: 11431 (97.5883 %)
Memory usage VmPeak: 119764 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:50:29 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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461136.74061653 06.04.2026 05:46:19.268 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 73
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 19 seconds
Number of parallel threads: 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): 85139
Objects passed selection criteria: 84950
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 65388
Average stars matched: 63143.2 (96.567 %)
Memory usage VmPeak: 2847464 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:52:10 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.73993561
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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits'
wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:20.345 +05:59:20.22
Angular distance between the image centers 0.0112 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:18.422 +05:59:12.55
Angular distance between the image centers 0.0055 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 08:34:20.345 +05:59:20.22
Second-epoch second image center 08:34:18.422 +05:59:12.55
Angular distance between the image centers 0.00825 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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.1fWwc4e4zt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.KoBkAn6XhA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits &> /tmp/tmp.HqpAmvORxb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits &> /tmp/tmp.z3hYmZqWDx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Read 15650 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.5654 to 136.5445 deg, Dec +0.6765 to +11.2689 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 120.5654 to 136.5445 deg, Dec 0.6765 to 11.2689 deg
Loaded 8720 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): 7106 out of 7589 total matches.
Matched with Tycho-2 7589 out of 15650 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955413
a=0.000000 b=1.000000 c=22.955413
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 20 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.3 pix Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
4.5 pix fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
4.5 pix fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Limiting magnitude estimates:
15.3 mag. Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.3 mag. Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
14.2 mag. fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
14.2 mag. fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.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.1fWwc4e4zt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=15650
Got 15650 stars (including 14444 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 15650 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 453 to 508 (Dec 0.7 to 11.3)
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...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15104 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.KoBkAn6XhA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=15565
Got 15565 stars (including 14349 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 15565 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15149 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.HqpAmvORxb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=589, passed=8023
Got 8023 stars (including 7430 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat
util/solve_plate_with_UCAC5 got 8023 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 7919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 7919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 7919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.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.z3hYmZqWDx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=593, passed=7970
Got 7970 stars (including 7372 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat
util/solve_plate_with_UCAC5 got 7970 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.7)
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...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 7842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 7843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 7843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 945 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits'
Preparing the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20974.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20756_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 20756_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:10:05.47 +06:20:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20757_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 20757_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:54:16.63 +02:36:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.259 578016702991453824 133.56860435124 +02.60289534818 11.4650 11.0053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20759_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 20759_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 20783_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 20783_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:02:49.14 +03:58:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.90, MAG_FAINT_SEARCH_LIMIT=9.88)GAIADR2_OUTPUT=# 0.077 3094420827491500288 120.70473298940 +03.96737431910 8.6312 7.8330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20804_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 20804_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:02:55.39 +02:43:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.46, MAG_FAINT_SEARCH_LIMIT=10.44)GAIADR2_OUTPUT=# 0.530 3093997481155271936 120.73089078976 +02.71889099250 9.3099 8.6865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20871_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 20871_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:14:18.95 +08:34:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20882_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 20882_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:35:01.94 +02:59:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20974_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 20974_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 06271_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 06271_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:40:13.10 +06:33:58.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 04296_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 04296_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:39:24.28 +08:01:01.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06180_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 06180_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:35:50.69 +06:37:12.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 08891_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 08891_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:33:43.41 +04:45:30.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 07433_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 07433_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:37:38.96 +05:42:17.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 04816_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 04816_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:25:55.00 +07:33:50.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 11020_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 11020_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:38:45.24 +03:20:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06384_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 06384_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:46:45.59 +06:25:08.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 07261_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 07261_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:48:25.30 +05:50:19.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 10957_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 10957_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:43:12.99 +03:24:05.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 07022_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 07022_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:55:22.88 +05:56:47.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 02565_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 02565_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:16:31.30 +09:11:03.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 17s
Prepared the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:37:12.40 +06:17:00.9
08:55:42.11 +08:55:33.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits exists and is non-empty
wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:20.345 +05:59:20.22
Angular distance between the image centers 0.0112 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:18.422 +05:59:12.55
Angular distance between the image centers 0.0055 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 08:34:20.345 +05:59:20.22
Second-epoch second image center 08:34:18.422 +05:59:12.55
Angular distance between the image centers 0.00825 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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.VvalZsDYer
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.ys2OhJSmkf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits &> /tmp/tmp.Jeepbb77Mu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits &> /tmp/tmp.FOEMyQ3BPb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Read 90472 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.5655 to 136.5508 deg, Dec +0.6702 to +11.2724 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 120.5655 to 136.5508 deg, Dec 0.6702 to 11.2724 deg
Loaded 8738 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): 6435 out of 7690 total matches.
Matched with Tycho-2 7690 out of 90472 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.847783
a=0.000000 b=1.000000 c=22.847783
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 64 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.1 pix Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
3.5 pix fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
3.5 pix fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Limiting magnitude estimates:
15.5 mag. Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.5 mag. Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
14.2 mag. fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
14.2 mag. fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.VvalZsDYer (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6373, passed=90453
Got 90453 stars (including 83928 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 90453 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 88129 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 88126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 88125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.ys2OhJSmkf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6475, passed=90928
Got 90928 stars (including 84300 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 90928 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 88620 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 88620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 88620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.Jeepbb77Mu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=3928, passed=41516
Got 41516 stars (including 37548 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat
util/solve_plate_with_UCAC5 got 41516 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 40899 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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 40897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 40896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 946 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.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.FOEMyQ3BPb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=3947, passed=41404
Got 41404 stars (including 37413 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat
util/solve_plate_with_UCAC5 got 41404 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 40836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 40835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 40834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 950 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-45-20_20.00sec_-4.90C_LIGHTs_0104.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Hya-01-Q1b1x1_004715_TTUQ1b1x1_28674_3G1vh0PY/wcs_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105.fits
Preparing the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out107223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out100750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46628.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 107217_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 107217_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 107223_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107223_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:11:24.76 +09:39:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.883 3146555030315414784 122.85447243912 +09.66265601272 13.4910 13.0209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107239_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 107239_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 107244_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107244_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 09:01:02.00 +09:55:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 5.205 603495067466402048 135.25692325765 +09.91929287500 13.6146 13.1589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107246_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107246_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:27:19.54 +10:30:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.728 600785041886578944 126.83120333213 +10.50134615680 13.4815 12.7886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107258_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107258_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:12:14.12 +08:15:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107267_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107267_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:08:06.39 +09:41:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107272_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107272_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:28:32.20 +01:29:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107279_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107279_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 107284_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107284_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:14:43.35 +04:07:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107285_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107285_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107291_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107291_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:09:14.15 +02:26:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107292_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107292_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:30:26.32 +10:31:27.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 107295_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107295_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:09:40.89 +10:12:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107296_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107296_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:59:59.50 +02:14:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.156 577021503233783808 134.99767203188 +02.24637471395 13.2012 12.6669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107298_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107298_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:49:37.47 +10:11:50.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 107300_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107300_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:13:00.25 +02:57:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107304_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 107304_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 107305_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107305_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:33:58.92 +08:11:08.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 107315_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107315_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:05:09.11 +09:07:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.260 3146250190716597376 121.28764394455 +09.11988369010 13.5752 13.2077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107316_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 107316_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 107317_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 107317_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 107319_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107319_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 107326_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107326_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:17:20.72 +01:59:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107331_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107331_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:26:33.02 +01:08:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107332_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107332_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:37:34.40 +02:09:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107335_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107335_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:36:06.17 +10:20:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107339_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107339_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 09:04:31.24 +06:07:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.881 583421936513306496 136.12972966522 +06.12587663543 12.7039 12.1917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107340_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107340_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:34:49.04 +01:17:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.564 3078598404193501184 128.70427142891 +01.29509905030 12.1225 11.6716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107341_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107341_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 09:03:29.83 +04:12:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107342_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107342_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:16:14.24 +02:46:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 3.811 3091194894733912576 124.06005931390 +02.76946560980 11.9786 11.2780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107343_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107343_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:14:13.04 +08:35:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107344_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107344_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:43:21.21 +00:58:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107345_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107345_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:10:05.42 +06:20:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107369_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107369_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:02:49.14 +03:58:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.91, MAG_FAINT_SEARCH_LIMIT=9.89)GAIADR2_OUTPUT=# 0.077 3094420827491500288 120.70473298940 +03.96737431910 8.6312 7.8330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107388_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107388_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:02:55.37 +02:43:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.46, MAG_FAINT_SEARCH_LIMIT=10.44)GAIADR2_OUTPUT=# 0.663 3093997481155271936 120.73089078976 +02.71889099250 9.3099 8.6865 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#
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Considering the candidate 107566_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107566_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:55:42.09 +08:55:33.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 107846_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107846_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:04:26.20 +11:06:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 3.991 3147890795207064960 121.10898342126 +11.11631604859 12.4471 11.8363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107950_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 107950_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:03:01.63 +01:27:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.112 3084844562250510080 120.75685148773 +01.45183075870 12.6121 11.9116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108082_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 108082_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:05:36.34 +11:07:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.194 3147722402426140416 121.40167886402 +11.12554272556 12.9575 12.4761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108197_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 108197_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:18:44.96 +01:57:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108264_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 108264_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 108507_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 108507_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:06:47.88 +01:24:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108543_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 108543_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:02:59.15 +01:59:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.987 3084948534818445952 120.74627445578 +01.98478686420 13.6442 13.2901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 30750_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 30750_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 09:02:44.35 +07:17:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 42187_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 42187_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:55:22.87 +05:56:47.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 46171_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 46171_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 09:01:30.94 +05:38:29.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 13235_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 13235_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:57:41.67 +09:23:14.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 08238_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 08238_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:44:44.68 +10:04:50.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 11605_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 11605_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:37:05.57 +09:39:16.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 81357_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 81357_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:43:13.00 +03:24:05.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 43037_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 43037_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:48:25.30 +05:50:18.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 38449_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 38449_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:46:45.59 +06:25:08.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 45870_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 45870_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:45:00.93 +05:40:52.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 24933_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 24933_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:39:24.28 +08:01:01.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65431_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 65431_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:33:43.41 +04:45:29.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 45164_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 45164_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:37:38.95 +05:42:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20546_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 20546_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:14:18.96 +08:34:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100750_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 100750_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 78550_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 78550_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:35:01.85 +02:59:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46628_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
Preparing report for the candidate 46628_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
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Considering the candidate 07583_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 07583_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:13:38.56 +10:11:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21300_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 21300_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
**** FOUND 08:34:13.28 +08:27:04.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 87976_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105
The candidate 87976_fd_Hya-01-Q1b1x1_2026-04-06_00-46-19_20.00sec_-5.00C_LIGHTs_0105 did not pass the final checks
