This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185142-0731.7,2461135.8983,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185142-0731.7 20260405.3982 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J281.6297-09.2218,2461135.8983,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J281.6297-09.2218 20260405.3982 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GV Sct,2461135.8983,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GV Sct 20260405.3982 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4253206336979410560,2461135.8983,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4253206336979410560 20260405.3982 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184933.54-104238.3,2461135.8983,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J184933.54-104238.3 20260405.3982 12.99CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4252507975255129856,2461135.8983,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4252507975255129856 20260405.3982 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J182654-0720.8,2461135.8983,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J182654-0720.8 20260405.3982 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4106980494464267136,2461135.8983,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4106980494464267136 20260405.3982 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4251930628560955904,2461135.8983,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4251930628560955904 20260405.3982 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LO Sct,2461135.8983,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LO Sct 20260405.3982 12.67CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4252731072987970944,2461135.8983,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4252731072987970944 20260405.3982 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184407-0733.0,2461135.8983,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184407-0733.0 20260405.3982 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J280.8542-07.2657,2461135.8983,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J280.8542-07.2657 20260405.3982 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4252731072987970944,2461135.8983,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4252731072987970944 20260405.3982 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184722-0910.1,2461135.8983,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184722-0910.1 20260405.3982 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4104807692068300288,2461135.8983,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4104807692068300288 20260405.3982 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4155992084269938432,2461135.8983,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4155992084269938432 20260405.3982 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461135.8983,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260405.3982 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4251723370641591040,2461135.8983,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4251723370641591040 20260405.3982 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461135.8983,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260405.3982 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461135.8983,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260405.3982 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461135.8983,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260405.3982 13.19CV 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: 2461118.93945891 19.03.2026 10:32:39.250 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
First image: 2461118.93945891 19.03.2026 10:32:39.250 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Last image: 2461135.89855041 05.04.2026 09:33:44.755 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.32
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): 11495
Objects passed selection criteria: 11463
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 9012.5
Average stars matched: 8719.75 (96.7517 %)
Memory usage VmPeak: 117648 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 04:43:20 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: 2461118.93945891 19.03.2026 10:32:39.250 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
First image: 2461118.93945891 19.03.2026 10:32:39.250 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Last image: 2461135.89855041 05.04.2026 09:33:44.755 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 184
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
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: 57 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): 147868
Objects passed selection criteria: 147639
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 121481
Average stars matched: 116472 (95.8771 %)
Memory usage VmPeak: 2113064 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 04:46:46 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
SExtractor catalog cache: saved Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat to cache
SExtractor catalog cache: saved Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.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/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.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: 2461135.89794995
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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits exists and is non-empty
Saving wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits to local_wcs_cache/
'wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits' -> 'local_wcs_cache/wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits'
wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits exists and is non-empty
Saving wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits to local_wcs_cache/
'wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits' -> 'local_wcs_cache/wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits'
wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits exists and is non-empty
Saving wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits to local_wcs_cache/
'wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits' -> 'local_wcs_cache/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits'
wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits exists and is non-empty
Saving wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits to local_wcs_cache/
'wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits' -> 'local_wcs_cache/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits'
The image scale is 5.88"/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 18:51:12.930 -10:02:01.64
Second-epoch image center 18:51:29.384 -10:00:09.01
Angular distance between the image centers 0.0744 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 18:51:12.930 -10:02:01.64
Second-epoch image center 18:51:32.490 -10:00:12.48
Angular distance between the image centers 0.0858 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 18:51:29.384 -10:00:09.01
Second-epoch second image center 18:51:32.490 -10:00:12.48
Angular distance between the image centers 0.01278 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/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits &> /tmp/tmp.Cu4UoXDTzF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits &> /tmp/tmp.AH40QRw48W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits &> /tmp/tmp.ZX01FGGr8n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits &> /tmp/tmp.DblRwpK89q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Calibrating the magnitude scale
Found non-empty wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits and wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits and wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
Found non-empty wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits and wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
The reference image (wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits) and catalog (wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat) found
'wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat' -> 'wcsmag.cat'
Read 14681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.6346 to 290.8039 deg, Dec -15.3419 to -4.6162 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 274.6346 to 290.8039 deg, Dec -15.3419 to -4.6162 deg
Loaded 14079 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): 8939 out of 9453 total matches.
Matched with Tycho-2 9453 out of 14681 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799591
a=0.000000 b=1.000000 c=22.799591
From vast_summary.log: estimated ref. image limiting mag.: -8.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
2.4 pix Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
2.6 pix fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
2.6 pix fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Limiting magnitude estimates:
14.5 mag. Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
14.5 mag. Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
13.7 mag. fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
13.7 mag. fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.0 (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.Cu4UoXDTzF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits' -> 'wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
WCS_IMAGE_NAME=wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
WCS-calibrated image found: wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Checking if the catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits alredy exist and is non-empty...
Catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
WCS catalog name: wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1205, passed=14681
Got 14681 stars (including 13457 good ones) from the SExtractor catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
util/solve_plate_with_UCAC5 got 14681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 428 (Dec -15.3 to -4.6)
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...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 14146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 14146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 14146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits -region wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.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.AH40QRw48W (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits' -> 'wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
Checking if the catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
WCS catalog name: wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1177, passed=14811
Got 14811 stars (including 13617 good ones) from the SExtractor catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 14811 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 14352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 14353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 14353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 950 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits -region wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.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.ZX01FGGr8n (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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
WCS_IMAGE_NAME=wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
WCS-calibrated image found: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
Checking if the catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits alredy exist and is non-empty...
Catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
WCS catalog name: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=539, passed=7019
Got 7019 stars (including 6472 good ones) from the SExtractor catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat
util/solve_plate_with_UCAC5 got 7019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 6804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 6804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 6804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 956 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits -region wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.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.DblRwpK89q (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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
WCS_IMAGE_NAME=wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
WCS-calibrated image found: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Checking if the catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits alredy exist and is non-empty...
Catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
WCS catalog name: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=7200
Got 7200 stars (including 6619 good ones) from the SExtractor catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat
util/solve_plate_with_UCAC5 got 7200 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 6970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 6969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 6969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
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_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits -region wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits'
Saving fully-calibrated image wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits'
Saving fully-calibrated image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits'
Saving fully-calibrated image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits'
Preparing the HTML report for the field Sct-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20987.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20987_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 20987_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:46:05.96 -06:38:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 0.492 4253141912460088192 281.52469643938 -06.63340204658 10.2711 9.4270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21095_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 21095_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Sct-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
SExtractor catalog cache: saved Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat to cache
SExtractor catalog cache: saved Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Creating symlink local_wcs_cache/wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
Creating symlink local_wcs_cache/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
Creating symlink local_wcs_cache/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits exists and is non-empty
wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits exists and is non-empty
wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits exists and is non-empty
wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits exists and is non-empty
The image scale is 5.88"/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 18:51:12.930 -10:02:01.64
Second-epoch image center 18:51:29.384 -10:00:09.01
Angular distance between the image centers 0.0744 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 18:51:12.930 -10:02:01.64
Second-epoch image center 18:51:32.490 -10:00:12.48
Angular distance between the image centers 0.0858 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 18:51:29.384 -10:00:09.01
Second-epoch second image center 18:51:32.490 -10:00:12.48
Angular distance between the image centers 0.01278 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/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits &> /tmp/tmp.feT09KYYM3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits &> /tmp/tmp.AxI7When3r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits &> /tmp/tmp.ixbYlijesc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits &> /tmp/tmp.HtOvFuIhND
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Calibrating the magnitude scale
Found non-empty wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits and wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits and wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
Found non-empty wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits and wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
The reference image (wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits) and catalog (wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat) found
'wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat' -> 'wcsmag.cat'
Read 184018 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.6118 to 290.8043 deg, Dec -15.3437 to -4.6093 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 274.6118 to 290.8043 deg, Dec -15.3437 to -4.6093 deg
Loaded 14107 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): 9184 out of 12312 total matches.
Matched with Tycho-2 12312 out of 184018 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.525476
a=0.000000 b=1.000000 c=22.525476
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 131 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
2.2 pix Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
2.2 pix fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
2.2 pix fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Limiting magnitude estimates:
14.6 mag. Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
14.6 mag. Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
13.8 mag. fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
13.8 mag. fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
All-image limiting magnitude estimate: 13.8 (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.feT09KYYM3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits' -> 'wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
WCS_IMAGE_NAME=wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
WCS-calibrated image found: wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Checking if the catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits alredy exist and is non-empty...
Catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
WCS catalog name: wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=24116, passed=183991
Got 183991 stars (including 159680 good ones) from the SExtractor catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat
util/solve_plate_with_UCAC5 got 183991 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 177442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 177442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 177444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 949 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits -region wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.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.AxI7When3r (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits' -> 'wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
Checking if the catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat corresponding to the image wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
WCS catalog name: wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=23603, passed=180864
Got 180864 stars (including 157082 good ones) from the SExtractor catalog wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 180864 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 428 (Dec -15.3 to -4.6)
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...
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 174334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 174333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 174331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits -region wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.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.ixbYlijesc (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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
WCS_IMAGE_NAME=wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
WCS-calibrated image found: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
Checking if the catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits alredy exist and is non-empty...
Catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
WCS catalog name: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=11, blended=7932, passed=94180
Got 94180 stars (including 86114 good ones) from the SExtractor catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat
util/solve_plate_with_UCAC5 got 94180 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 429 (Dec -15.3 to -4.6)
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...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 91709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 91706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 91706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 956 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits -region wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.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.HtOvFuIhND (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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
WCS_IMAGE_NAME=wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
WCS-calibrated image found: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Checking if the catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits alredy exist and is non-empty...
Catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
WCS catalog name: wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=8186, passed=95706
Got 95706 stars (including 87389 good ones) from the SExtractor catalog wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat
util/solve_plate_with_UCAC5 got 95706 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 373 to 429 (Dec -15.3 to -4.6)
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...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 92201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 92200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 92201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 958 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits -region wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits
Saving fully-calibrated image wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_Sct-01-Q2b1x1_2026-03-19_05-33-50_20.00sec_-14.90C_LIGHT_0191.fits
Saving fully-calibrated image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-32-52_20.00sec_-5.00C_LIGHT_0195.fits
Saving fully-calibrated image wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.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_2026-04-05_CI_Sct-01-Q2b1x1_043543_TTUQ2b1x1_28711_Hrq0llrk/wcs_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196.fits
Preparing the HTML report for the field Sct-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out139439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out211450.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out212022.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out211296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212829.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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: 15s
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Considering the candidate 211199_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211199_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:00:17.93 -12:41:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.157 4198559234589560704 285.07456706045 -12.69657079700 13.4989 12.8294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211201_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211201_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:58:07.00 -11:55:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.954 4198849574382939776 284.52837902189 -11.93063448829 13.7039 12.7566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211225_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211225_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:15:14.84 -10:04:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211227_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211227_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:01:37.80 -14:01:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 211228_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211228_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:04:07.64 -08:48:15.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 211232_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211232_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:45:57.28 -11:26:19.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 211242_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211242_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:58:20.86 -11:36:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.544 4198894031549236352 284.58685269040 -11.60280416584 12.7643 11.6985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211252_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211252_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:54:03.77 -11:12:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.633 4202149964716433408 283.51553286313 -11.19999185483 13.3779 12.8383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211259_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211259_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:27:06.28 -10:23:46.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 211260_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211260_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:42:03.31 -06:22:26.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 211279_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211279_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:00:20.22 -06:46:29.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
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Considering the candidate 211281_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211281_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:05:42.22 -06:10:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.738 4206120262485219712 286.42663854095 -06.17711074255 12.1086 10.8000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211283_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211283_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:34:07.07 -14:16:57.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 211286_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211286_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:44:33.29 -05:59:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.015 4253415789515869568 281.13926547662 -05.98889397252 12.9192 12.5471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211296_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211296_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211297_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211297_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:13:48.08 -07:34:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.015 4204788066711262848 288.45039363598 -07.56697432868 13.3524 12.5024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211298_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211298_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:45:16.94 -08:56:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.692 4251457254461567232 281.32008230208 -08.93733177692 11.2865 9.9748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211300_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211300_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:06:43.06 -08:49:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211301_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211301_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:56:30.39 -11:50:44.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 211304_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211304_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:15:50.44 -08:18:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.029 4201683874823653632 288.96044705095 -08.30609663388 13.4839 12.6525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211307_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211307_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211312_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211312_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:37:30.55 -07:44:16.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 211324_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211324_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:55:48.36 -12:14:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.315 4102769060030448384 283.95158858480 -12.24868122722 12.9099 11.9293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211325_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211325_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:02:58.49 -14:01:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211327_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211327_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:59:18.61 -13:45:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.608 4102359526299406080 284.82757908740 -13.75644357490 12.9268 12.0713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211344_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211344_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:15:28.98 -10:15:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211345_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211345_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:39:30.26 -10:05:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.914 4155240984759674624 279.87550843956 -10.09043983026 11.2890 9.9737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211347_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211347_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211348_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211348_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:03:00.67 -11:22:37.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 211349_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211349_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:46:34.97 -07:25:14.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 211353_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211353_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:34:15.35 -13:36:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.345 4104584040165854720 278.56433136422 -13.61138144979 12.4488 11.8502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211354_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211354_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:04:29.48 -11:51:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.308 4198732403344385792 286.12270217471 -11.86421569203 13.1076 12.5043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211364_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211364_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211368_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211368_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:04:40.77 -11:32:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.349 4198760131648829568 286.16960488678 -11.54562376350 12.8823 11.9531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211369_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211369_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211371_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211371_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:52:32.29 -06:59:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.687 4252225984881346432 283.13542835326 -06.98544030907 12.5476 11.5664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211372_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211372_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:50:08.24 -07:54:37.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
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Considering the candidate 211383_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211383_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:41:43.45 -06:18:36.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
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Considering the candidate 211384_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211384_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:41:38.48 -07:12:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.836 4252747153394380800 280.41044987060 -07.20719604046 10.2622 8.7788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211390_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211390_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:13:49.40 -10:48:34.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 211393_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211393_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211395_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211395_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:52:08.61 -06:38:44.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 211397_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211397_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:28:33.44 -09:07:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.525 4156149142634542976 277.14026999058 -09.11995632129 11.1181 9.8120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211400_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211400_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:35:55.65 -13:41:18.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 211401_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211401_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:43:04.30 -07:29:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 211402_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211402_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211405_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211405_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:43:28.27 -08:01:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211407_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211407_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211409_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211409_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:44:02.74 -06:07:23.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
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Considering the candidate 211411_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211411_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:55:00.43 -06:11:20.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 211412_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211412_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:49:26.56 -12:38:33.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 211414_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211414_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211420_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211420_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:01:11.80 -08:49:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211421_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211421_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211429_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211429_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:56:48.66 -06:52:21.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)
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Considering the candidate 211433_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211433_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:33:18.03 -11:57:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.939 4153073812931109120 278.32507377700 -11.95636964110 12.4689 11.8689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211435_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211435_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:13:33.81 -11:27:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.999 4198397331484829568 288.39059181219 -11.46555936043 12.9303 12.1286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211440_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211440_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:02:48.51 -13:59:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.979 4101554134030539904 285.70186173547 -13.98818470517 12.6199 11.9069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211441_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211441_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211446_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211446_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211447_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211447_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211448_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211448_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:52:55.28 -05:43:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211450_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211450_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:23:37.96 -06:04:10.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 211452_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211452_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 211458_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211458_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:11:38.36 -08:55:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.615 4201252007275468160 287.90969848191 -08.93118268729 12.8094 11.8271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211459_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211459_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211460_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211460_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:43:37.18 -07:56:42.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 211465_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211465_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:50:49.57 -06:06:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 3.215 4252518901680682368 282.70670644673 -06.10829464649 12.5072 12.1273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211466_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211466_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:14:56.05 -09:54:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.729 4200896177818966528 288.73334382539 -09.90022325237 12.7175 12.1148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211476_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211476_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:43:21.05 -07:23:51.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)
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Considering the candidate 211477_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211477_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:44:52.26 -06:05:50.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)
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Considering the candidate 211479_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211479_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:51:18.04 -14:03:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211486_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211486_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:32:50.27 -07:01:44.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)
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Considering the candidate 211487_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211487_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:30:26.76 -13:51:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.581 4104374858074460800 277.61164772574 -13.85617590258 12.5646 11.9253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211494_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211494_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211496_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211496_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:34:58.13 -13:05:51.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
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Considering the candidate 211497_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211497_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:43:32.75 -07:26:17.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)
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Considering the candidate 211498_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211498_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211500_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211500_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:15:54.08 -07:44:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.448 4204814351917637120 288.97525584661 -07.73548665669 12.2988 11.7573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211503_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211503_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:42:44.19 -06:15:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.745 4253382568021228032 280.68508357772 -06.26580464460 10.9869 9.7160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211504_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211504_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:14:18.62 -08:26:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.791 4201655523722539776 288.57754303692 -08.43889505935 11.8995 11.0410 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 211508_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211508_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:48:44.64 -07:06:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 1.898 4252302538408300416 282.18647071707 -07.11354995800 11.3866 10.4315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211510_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211510_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:30:35.59 -13:40:53.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)
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Considering the candidate 211511_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211511_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:45:43.64 -06:49:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211512_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211512_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211515_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211515_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:14:44.96 -09:56:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211520_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211520_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:07:31.27 -12:51:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.213 4197805102720899328 286.88027749018 -12.85061302860 11.9450 11.0864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211523_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211523_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:49:15.26 -07:10:41.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)
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Considering the candidate 211525_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211525_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:40:59.00 -06:46:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211526_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211526_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:24:05.97 -11:22:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 4.586 4154058082002792960 276.02608149827 -11.38094340697 10.7532 9.9012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211527_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211527_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:10:04.23 -09:01:21.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)
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Considering the candidate 211651_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 211651_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 211744_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211744_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:08:03.46 -08:45:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 1.014 4204226113188551040 287.01430381666 -08.75553651920 11.4136 10.5412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211766_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211766_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:02:37.59 -13:49:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 0.856 4101572207253151104 285.65638039789 -13.82490446997 11.6595 10.8654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211833_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 211833_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:13:42.83 -10:38:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.525 4200735546040913024 288.42803620139 -10.64358573748 12.2914 11.8610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212011_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212011_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 212022_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212022_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:25:22.53 -12:32:06.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)
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Considering the candidate 212039_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212039_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:15:57.07 -10:01:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212132_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212132_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:42:30.65 -07:03:42.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212192_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212192_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:55:57.14 -10:59:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212239_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212239_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:15:28.20 -11:45:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212275_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212275_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:42:25.50 -07:19:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212298_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212298_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:04:29.79 -10:38:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 2.275 4199436090784186368 286.12463534339 -10.64767111035 12.2000 11.0486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212338_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 212338_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 212339_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212339_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:43:39.31 -08:23:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212340_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212340_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:02:16.42 -08:03:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212346_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212346_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:56:29.71 -11:19:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212372_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212372_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:07:50.17 -10:37:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.820 4199469866408016512 286.95852753532 -10.62748705012 13.0991 12.1811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212411_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212411_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:07:46.66 -13:02:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.230 4197781291428476544 286.94555320185 -13.04271759846 12.6563 11.6408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212529_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212529_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:15:43.21 -08:33:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212563_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 212563_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 212604_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212604_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:05:40.96 -12:00:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.207 4198677805721357824 286.42100914958 -12.01342813770 13.6735 12.7211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212692_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212692_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:08:04.48 -07:52:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212701_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 212701_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 212718_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212718_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:55:39.53 -13:51:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.067 4102299087525908608 283.91444388843 -13.86262971036 13.0540 12.3530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212745_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212745_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:01:21.53 -13:39:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.671 4101636318203344640 285.33869041090 -13.66408075862 12.2963 10.9117 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212763_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212763_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:14:29.86 -10:33:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.262 4199993199585076480 288.62444697053 -10.56501584419 13.3366 12.5526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212805_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212805_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:58:34.92 -09:08:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212829_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
Preparing report for the candidate 212829_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
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Considering the candidate 212854_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212854_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:42:48.67 -08:18:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.843 4251740172555664640 280.70291015292 -08.30925178790 12.5887 11.7240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212872_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212872_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:14:06.12 -07:59:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.635 4204713059408002048 288.52546913634 -07.98443726114 13.3010 12.3916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212915_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 212915_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:09:06.92 -13:37:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.642 4197423988824697344 287.27915817753 -13.62178174172 13.5972 12.6767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213062_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 213062_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:07:33.20 -13:22:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.812 4197493425542544000 286.88781850782 -13.37935517433 13.7646 13.0810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213094_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 213094_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:12:17.99 -08:54:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.996 4201241836793229824 288.07541243321 -08.90950744014 13.3655 12.5192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213101_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 213101_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:07:49.91 -14:08:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.349 4197369799199603584 286.95731270943 -14.13640565157 13.9241 13.2488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213168_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 213168_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:07:11.03 -12:51:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213209_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 213209_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:08:42.48 -13:48:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 0.826 4197417597912841088 287.17679041538 -13.80602229528 14.0704 13.4407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213260_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 213260_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 19:14:35.93 -11:28:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139439_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 139439_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:55:26.76 -07:18:23.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)
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Considering the candidate 68776_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 68776_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
**** FOUND 18:39:28.56 -11:12:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136874_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196
The candidate 136874_fd_Sct-01-Q2b1x1_2026-04-05_04-33-44_20.00sec_-5.00C_LIGHT_0196 did not pass the final checks
