This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6276905999421273856,2461139.7646,11.47,0.05,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 6276905999421273856 20260409.2646 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J140114-2614.1,2461139.7646,10.29,0.05,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
ASAS J140114-2614.1 20260409.2646 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J141438-2615.3,2461139.7646,9.55,0.05,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
ASAS J141438-2615.3 20260409.2646 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6175269519668010752,2461139.7646,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6175269519668010752 20260409.2646 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.7646,12.90,0.05,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 20260409.2646 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6176785196446507008,2461139.7646,12.57,0.05,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 6176785196446507008 20260409.2646 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J224.4110-29.0463,2461139.7646,12.27,0.05,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 J224.4110-29.0463 20260409.2646 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6205819106651026048,2461139.7646,12.15,0.05,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 6205819106651026048 20260409.2646 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6217944589603275904,2461139.7646,12.00,0.05,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 6217944589603275904 20260409.2646 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7646,13.15,0.05,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 20260409.2646 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J143012-2645.7,2461139.7646,11.90,0.05,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
ASAS J143012-2645.7 20260409.2646 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J144106-2517.2,2461139.7646,9.37,0.05,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
ASAS J144106-2517.2 20260409.2646 9.37CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J141947-2902.1,2461139.7646,10.67,0.05,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
ASAS J141947-2902.1 20260409.2646 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J143604-2326.4,2461139.7646,11.18,0.05,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
ASAS J143604-2326.4 20260409.2646 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J140855-2645.7,2461139.7646,11.68,0.05,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
ASAS J140855-2645.7 20260409.2646 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J143137-2829.5,2461139.7646,10.99,0.05,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
ASAS J143137-2829.5 20260409.2646 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J141720.80-230633.2,2461139.7646,12.38,0.05,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
ASASSN-V J141720.80-230633.2 20260409.2646 12.38CV 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: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
First image: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Last image: 2461139.76494976 09.04.2026 06:21:21.659 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 31
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.22
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): 7168
Objects passed selection criteria: 7156
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 6350.5
Average stars matched: 6197 (97.5829 %)
Memory usage VmPeak: 112816 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:23:21 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: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
First image: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Last image: 2461139.76494976 09.04.2026 06:21:21.659 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 63
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
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): 44463
Objects passed selection criteria: 44387
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 36140.2
Average stars matched: 34895 (96.5544 %)
Memory usage VmPeak: 146296 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:24:47 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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
SExtractor catalog cache: saved Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat to cache
SExtractor catalog cache: saved Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.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: 2461139.76425625
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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits exists and is non-empty
Saving wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits to local_wcs_cache/
'wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> 'local_wcs_cache/wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits exists and is non-empty
Saving wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits to local_wcs_cache/
'wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> 'local_wcs_cache/wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits exists and is non-empty
Saving wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits to local_wcs_cache/
'wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits' -> 'local_wcs_cache/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits'
wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
Saving wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits to local_wcs_cache/
'wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'local_wcs_cache/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:24:09.002 -25:59:19.42
Second-epoch image center 14:23:57.953 -25:59:06.78
Angular distance between the image centers 0.0415 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 14:24:09.002 -25:59:19.42
Second-epoch image center 14:23:59.256 -25:59:54.06
Angular distance between the image centers 0.0377 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 14:23:57.953 -25:59:06.78
Second-epoch second image center 14:23:59.256 -25:59:54.06
Angular distance between the image centers 0.01401 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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits &> /tmp/tmp.O2plfWbXaZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits &> /tmp/tmp.UMo8JRArf6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits &> /tmp/tmp.pvT5Zl0NWe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.kWanOBT19e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
Found non-empty wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
The reference image (wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits) and catalog (wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat) found
'wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat' -> 'wcsmag.cat'
Read 7306 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 206.8784 to 225.0225 deg, Dec -31.2717 to -20.4641 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 206.8784 to 225.0225 deg, Dec -31.2717 to -20.4641 deg
Loaded 7631 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): 5349 out of 5503 total matches.
Matched with Tycho-2 5503 out of 7306 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.777156
a=0.000000 b=1.000000 c=22.777156
From vast_summary.log: estimated ref. image limiting mag.: -8.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
2.4 pix Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
5.1 pix fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
5.1 pix fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Limiting magnitude estimates:
14.6 mag. Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
14.5 mag. Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
13.6 mag. fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
13.6 mag. fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.4 (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.O2plfWbXaZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> 'wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Checking if the catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS catalog name: wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=484, passed=7306
Got 7306 stars (including 6818 good ones) from the SExtractor catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 7306 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits -region wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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.UMo8JRArf6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> 'wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Checking if the catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS catalog name: wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=477, passed=7284
Got 7284 stars (including 6803 good ones) from the SExtractor catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 7284 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 7115 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 7112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 7112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits -region wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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.pvT5Zl0NWe (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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
Checking if the catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
WCS catalog name: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=216, passed=5451
Got 5451 stars (including 5233 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat
util/solve_plate_with_UCAC5 got 5451 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 5373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits -region wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.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.kWanOBT19e (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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=233, passed=5530
Got 5530 stars (including 5296 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat
util/solve_plate_with_UCAC5 got 5530 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 5451 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 5450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 5450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 954 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_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
Saving fully-calibrated image wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
Saving fully-calibrated image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits'
Saving fully-calibrated image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits'
Preparing the HTML report for the field Hya-14-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out05696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20497.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 20401_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20401_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:56:45.28 -25:32:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20412_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20412_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:13:32.77 -29:54:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20445_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20445_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:48:23.86 -27:15:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20450_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20450_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:02:04.12 -23:35:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 3.778 6275497490665977984 210.51817050615 -23.59252263571 11.4965 11.0066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20457_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20457_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:13:49.57 -23:32:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 1.074 6276083740818128768 213.45659073002 -23.54778850811 10.5435 9.1633 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20487_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20487_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:02:21.89 -21:16:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 1.203 6289375393288725504 210.59102344846 -21.27613022126 11.0398 9.9213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20497_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 20497_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 20501_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20501_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:13:03.56 -21:11:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.686 6277557704874751488 213.26463559136 -21.18543732634 11.6542 11.2232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20507_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20507_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:17:54.85 -23:18:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 0.430 6275965470303142912 214.47866524439 -23.31092624065 11.2769 10.2772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20523_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20523_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:22:08.70 -20:55:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 0.258 6282875213688380416 215.53617338479 -20.93010846905 11.7523 11.1664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20524_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20524_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:13:13.60 -21:00:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 0.238 6277749530998622720 213.30659636223 -21.00488162664 11.7728 11.3428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20525_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20525_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:04:30.09 -21:21:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 0.555 6289336459409234944 211.12521029491 -21.35062470356 11.7126 11.0155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20526_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20526_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:47:29.12 -22:07:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.211 6278763972209882880 221.87133137990 -22.13028069121 11.6031 10.8226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20536_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20536_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:17:14.12 -21:13:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 0.838 6277601474885632000 214.30858415333 -21.22995542571 11.8980 11.3393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20537_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20537_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:03:15.14 -22:31:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 0.640 6275736497006346880 210.81295830885 -22.51891281998 11.8208 11.3583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20538_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20538_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:34:57.74 -21:08:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 0.589 6279995489655986944 218.74074591680 -21.14920036555 11.6565 10.8324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20539_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20539_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:09:07.79 -20:43:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 0.968 6289464724312561536 212.28220994171 -20.73171860155 11.8215 11.3892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20542_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20542_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:56:55.27 -20:56:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 0.207 6288893150064893184 209.23033616771 -20.93520635375 11.8921 11.3562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20544_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20544_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:04:52.07 -21:09:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 0.757 6289344946265146240 211.21679180850 -21.15714188117 11.8246 11.3684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20547_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20547_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:58:25.09 -22:35:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 0.394 6287694304433564416 209.60447803149 -22.59268551524 11.6354 10.7052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20548_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20548_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:57:04.97 -21:12:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 0.359 6288110881902046976 209.27069305706 -21.20076542438 11.8720 11.3695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20549_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20549_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:56:37.67 -20:30:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 0.318 6288924073829418752 209.15697444210 -20.51521847806 11.8713 11.1537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20551_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20551_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:11:52.00 -22:01:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.345 6277114975350206976 212.96662114550 -22.02110837866 11.7899 11.2889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20553_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20553_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:13:17.13 -21:09:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.192 6277558185911014144 213.32131846431 -21.15921477057 11.6681 10.8317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20554_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20554_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:04:04.09 -21:45:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 0.276 6289290146778013824 211.01703128380 -21.76584059298 11.7822 11.0826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20555_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20555_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:08:23.54 -21:41:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.643 6277337076699381760 212.09792367955 -21.69965500650 11.8876 11.4532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20556_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 20556_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:59:38.81 -20:56:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 0.791 6289630544409932928 209.91150844332 -20.93972717621 11.9197 11.5035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 03809_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 03809_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 03883_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 03883_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 05696_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 05696_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:36:03.42 -23:26:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 1.341 6278341446210709760 219.01447869705 -23.44002556373 9.6680 8.2363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 19s
Prepared the HTML report for the field Hya-14-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 ####
14:01:13.91 -26:14:05.8
14:14:38.18 -26:15:16.1
14:09:48.87 -22:59:53.4
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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
SExtractor catalog cache: saved Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat to cache
SExtractor catalog cache: saved Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Creating symlink local_wcs_cache/wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits exists and is non-empty
wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits exists and is non-empty
wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits exists and is non-empty
wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:24:09.002 -25:59:19.42
Second-epoch image center 14:23:57.953 -25:59:06.78
Angular distance between the image centers 0.0415 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 14:24:09.002 -25:59:19.42
Second-epoch image center 14:23:59.256 -25:59:54.06
Angular distance between the image centers 0.0377 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 14:23:57.953 -25:59:06.78
Second-epoch second image center 14:23:59.256 -25:59:54.06
Angular distance between the image centers 0.01401 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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits &> /tmp/tmp.Jj7ZfIjVLp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits &> /tmp/tmp.dMNNvFw4IY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits &> /tmp/tmp.uNdoyz18jo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.vPf58we48v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
Found non-empty wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
The reference image (wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits) and catalog (wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat) found
'wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat' -> 'wcsmag.cat'
Read 48077 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 206.8452 to 225.0425 deg, Dec -31.2754 to -20.4430 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 206.8452 to 225.0425 deg, Dec -31.2754 to -20.4430 deg
Loaded 7679 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): 5937 out of 6447 total matches.
Matched with Tycho-2 6447 out of 48077 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.599077
a=0.000000 b=1.000000 c=22.599077
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.67
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.67
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
2.3 pix Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
4.5 pix fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
4.4 pix fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Limiting magnitude estimates:
14.7 mag. Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
14.7 mag. Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
13.9 mag. fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
13.9 mag. fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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.Jj7ZfIjVLp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> 'wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Checking if the catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS catalog name: wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2143, passed=48066
Got 48066 stars (including 45850 good ones) from the SExtractor catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 48066 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 46944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 46941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 46941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits -region wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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.dMNNvFw4IY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> 'wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Checking if the catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS catalog name: wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2237, passed=47980
Got 47980 stars (including 45682 good ones) from the SExtractor catalog wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 47980 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 46981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 46980 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 46980 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits -region wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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.uNdoyz18jo (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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
Checking if the catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
WCS catalog name: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1481, passed=24746
Got 24746 stars (including 23248 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat
util/solve_plate_with_UCAC5 got 24746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 24476 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 24477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 24477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits -region wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.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.vPf58we48v (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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat corresponding to the image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1513, passed=25376
Got 25376 stars (including 23850 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat
util/solve_plate_with_UCAC5 got 25376 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 25136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 25136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 25136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.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-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_Hya-14-Q1b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Saving fully-calibrated image wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_Hya-14-Q1b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Saving fully-calibrated image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-20-21_20.00sec_-4.90C_LIGHTs_0161.fits
Saving fully-calibrated image wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.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_2026-04-09_CI_Hya-14-Q1b1x1_012212_TTUQ1b1x1_2606_yDQbq7KC/wcs_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162.fits
Preparing the HTML report for the field Hya-14-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out10493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54540.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 8s
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Considering the candidate 53962_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 53962_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:41:42.76 -27:00:21.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)
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Considering the candidate 53969_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 53969_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:53:16.09 -21:57:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.344 6287964513712017280 208.31702705042 -21.96296098146 13.1520 12.5023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53974_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 53974_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:50:36.93 -23:06:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.191 6230408722130754176 222.65366872775 -23.10081222530 13.1552 12.6591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53989_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 53989_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:49:32.28 -28:48:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53991_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 53991_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 53992_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 53992_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 54000_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54000_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:18:43.73 -29:11:05.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
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Considering the candidate 54004_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 54004_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 54006_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 54006_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 54015_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 54015_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 54016_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 54016_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 54232_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54232_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:17:09.94 -21:46:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 1.652 6276734582982238080 214.29092271568 -21.77186893002 11.9168 11.0648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54249_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54249_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:36:05.40 -22:11:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.870 6279321871280373248 219.02331846936 -22.19991414949 11.7820 10.7432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54257_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54257_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:04:24.79 -21:45:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.825 6289287393704107776 211.10320764916 -21.76122910268 12.1359 11.4698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54281_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54281_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:19:45.23 -20:53:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.882 6277634013557854720 214.93820915590 -20.88896539033 12.2888 11.6829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54294_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54294_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:47:51.62 -26:39:37.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54339_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54339_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:11:10.69 -22:00:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.791 6277117968942929536 212.79468437353 -22.00936853358 12.8055 12.2795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54388_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54388_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:27:33.17 -22:01:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.674 6279516205667199360 216.88821972579 -22.01740915943 12.6419 11.8890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54397_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54397_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:30:26.63 -21:31:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.163 6279643031756084480 217.61124756369 -21.52320378454 12.8124 12.1683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54419_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54419_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:03:19.89 -24:48:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.807 6274073318166680064 210.83278149597 -24.80920743552 12.4759 11.7582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54461_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54461_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:12:54.58 -21:42:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.133 6277149232009348224 213.22734380980 -21.71461294208 13.1868 12.6807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54519_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54519_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:07:55.43 -22:10:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.358 6277215310081745280 211.98085327000 -22.17225663367 12.9398 12.2492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54521_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54521_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:22:02.49 -21:38:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.256 6276786942927632896 215.51031504300 -21.63462769805 13.3248 13.0399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54540_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 54540_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 54542_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54542_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:56:01.27 -26:42:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.932 6225565162955376768 224.00681314839 -26.71071706536 12.6477 10.6246 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54562_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54562_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:28:58.85 -25:19:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.275 6271543685509218304 217.24469999922 -25.32594191840 13.4229 12.9259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54645_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54645_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:52:32.43 -21:25:33.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 54648_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54648_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:06:28.63 -20:53:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.637 6289449198006948608 211.62031895970 -20.89710130395 14.0043 13.5166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54671_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54671_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:20:35.66 -20:52:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.986 6276889854639827968 215.14830372113 -20.87488781589 13.7384 13.1811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54688_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54688_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:54:29.79 -20:44:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.777 6288938990251811584 208.62429130680 -20.74128851480 13.8157 13.2622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54718_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 54718_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:00:05.02 -23:12:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 4.502 6275571918155440512 210.02012754936 -23.21462988102 14.0967 13.4829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07991_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 07991_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:28:10.30 -29:29:26.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22464_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 22464_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 08608_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 08608_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:53:32.95 -29:05:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23706_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 23706_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:01:13.91 -26:14:05.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 05438_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 05438_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:18:47.37 -30:05:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27046_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 27046_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 13:56:45.29 -25:32:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06066_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 06066_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:13:32.76 -29:54:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29307_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 29307_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 19554_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 19554_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:48:23.85 -27:15:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10493_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 10493_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 42665_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 42665_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 21789_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 21789_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 13513_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 13513_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 41512_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
Preparing report for the candidate 41512_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
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Considering the candidate 24356_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 24356_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:14:38.17 -26:15:16.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 16039_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 16039_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:23:05.45 -27:45:16.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 18767_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 18767_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:12:46.35 -27:15:41.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 02255_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 02255_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
**** FOUND 14:33:09.72 -30:42:55.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14767_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162
The candidate 14767_fd_Hya-14-Q1b1x1_2026-04-09_01-21-21_20.00sec_-4.90C_LIGHTs_0162 did not pass the final checks
