This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj
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
V0567 Aql,2461132.8865,10.24,0.05,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
V0567 Aql 20260402.3865 10.24CV 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 4299185679747173888,2461132.8865,12.57,0.05,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 4299185679747173888 20260402.3865 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461132.8865,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260402.3865 12.65CV 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
NSV 12186,2461132.8865,12.33,0.05,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
NSV 12186 20260402.3865 12.33CV 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
V0540 Aql,2461132.8865,12.28,0.05,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
V0540 Aql 20260402.3865 12.28CV 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
V1321 Aql,2461132.8865,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1321 Aql 20260402.3865 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193000.80+064952.3,2461132.8865,12.81,0.05,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 J193000.80+064952.3 20260402.3865 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0434 Aql,2461132.8865,11.85,0.05,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
V0434 Aql 20260402.3865 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
V0400 Aql,2461132.8865,11.68,0.05,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
V0400 Aql 20260402.3865 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J195913+0927.3,2461132.8865,11.11,0.05,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 J195913+0927.3 20260402.3865 11.11CV 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 J200142.54+090833.9,2461132.8865,12.21,0.05,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 J200142.54+090833.9 20260402.3865 12.21CV 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 J195157.71+084254.6,2461132.8865,12.10,0.05,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 J195157.71+084254.6 20260402.3865 12.10CV 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
V0438 Aql,2461132.8865,12.68,0.05,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
V0438 Aql 20260402.3865 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461132.88682443 02.04.2026 09:16:51.631 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15487
Objects passed selection criteria: 15437
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: 12066.2
Average stars matched: 11756.5 (97.4329 %)
Memory usage VmPeak: 121308 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:27:00 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461132.88682443 02.04.2026 09:16:51.631 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 127
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 59 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): 178478
Objects passed selection criteria: 178028
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 134772
Average stars matched: 129425 (96.0326 %)
Memory usage VmPeak: 2009864 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:32:51 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.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: 2461132.88611807
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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits'
wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:52.042 +05:59:42.52
Angular distance between the image centers 0.01 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 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:50.908 +05:59:11.29
Angular distance between the image centers 0.02 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 19:42:52.042 +05:59:42.52
Second-epoch second image center 19:42:50.908 +05:59:11.29
Angular distance between the image centers 0.00987 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.YvzhU6pGWZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.cDwrrcYlkk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits &> /tmp/tmp.6A8439Ft4H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.gsWaDR3Kmh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
The reference image (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat) found
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat' -> 'wcsmag.cat'
Read 19279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.6603 to 303.6488 deg, Dec +0.6156 to +11.3108 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 287.6603 to 303.6488 deg, Dec 0.6156 to 11.3108 deg
Loaded 16831 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): 11809 out of 12562 total matches.
Matched with Tycho-2 12562 out of 19279 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779826
a=0.000000 b=1.000000 c=22.779826
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
2.8 pix fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
2.8 pix fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Limiting magnitude estimates:
14.7 mag. Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
14.7 mag. Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
13.7 mag. fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
13.7 mag. fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.1 (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.YvzhU6pGWZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1674, passed=19279
Got 19279 stars (including 17574 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 19279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 964 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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.cDwrrcYlkk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1629, passed=19357
Got 19357 stars (including 17702 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 19357 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 965 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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.6A8439Ft4H (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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=501, passed=8242
Got 8242 stars (including 7738 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 8242 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.82"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.82"
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.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.gsWaDR3Kmh (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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=494, passed=8274
Got 8274 stars (including 7778 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 8274 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.83"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.84"
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 966 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
Saving fully-calibrated image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits'
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out03980.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 21232_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 21232_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:50:59.42 +08:51:12.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21235_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 21235_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:40:43.09 +09:55:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21237_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 21237_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:57:29.12 +08:42:24.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06780_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 06780_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:45:09.78 +04:54:22.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03980_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 03980_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Aql-02-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 ####
19:59:42.56 +03:18:40.8
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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:52.042 +05:59:42.52
Angular distance between the image centers 0.01 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 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:50.908 +05:59:11.29
Angular distance between the image centers 0.02 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 19:42:52.042 +05:59:42.52
Second-epoch second image center 19:42:50.908 +05:59:11.29
Angular distance between the image centers 0.00987 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.UAQJlDvajN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.0rWaCZzmGO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits &> /tmp/tmp.WmOiZV2y13
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.g3h9xKsgaj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
The reference image (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat) found
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat' -> 'wcsmag.cat'
Read 215901 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.6445 to 303.6494 deg, Dec +0.6156 to +11.3131 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 287.6445 to 303.6494 deg, Dec 0.6156 to 11.3131 deg
Loaded 16852 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): 11183 out of 14938 total matches.
Matched with Tycho-2 14938 out of 215901 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.584750
a=0.000000 b=1.000000 c=22.584750
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.88
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.88
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 81 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
2.6 pix fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
2.6 pix fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Limiting magnitude estimates:
14.9 mag. Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
14.9 mag. Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
13.8 mag. fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
13.8 mag. fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (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.UAQJlDvajN (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=26960, passed=215867
Got 215867 stars (including 188619 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 215867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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.0rWaCZzmGO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=27226, passed=216980
Got 216980 stars (including 189460 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 216980 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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.WmOiZV2y13 (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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=5750, passed=75284
Got 75284 stars (including 69461 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 75284 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.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.g3h9xKsgaj (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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=5786, passed=75517
Got 75517 stars (including 69644 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 75517 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 967 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Saving fully-calibrated image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-15-50_20.00sec_-14.90C_LIGHT_0040.fits
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.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_2026-04-02_CI_Aql-02-Q2b1x1_042059_TTUQ2b1x1_9629_cfVa8BPj/wcs_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041.fits
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out228472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out125061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73278.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 246995_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 246995_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:20:14.10 +09:40:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 246998_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 246998_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:36:29.83 +08:32:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247007_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247007_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:49:52.20 +09:29:16.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 247010_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247010_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:17:18.49 +09:29:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247025_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247025_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:28:49.41 +07:57:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.725 4295971601143608192 292.20536918474 +07.95448358892 13.0958 12.2003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247027_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247027_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:52:54.05 +10:16:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.921 4303250264998824704 298.22418027563 +10.27020898097 12.7318 12.2135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247028_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247028_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:25:02.35 +01:38:48.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)
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Considering the candidate 247029_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247029_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:36:15.58 +02:03:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247030_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 247030_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 247033_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247033_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:42:54.43 +09:53:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247034_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247034_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:59:42.50 +03:07:49.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)
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Considering the candidate 247035_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247035_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:33:39.75 +07:39:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247038_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 247038_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 247043_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247043_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:47:41.12 +09:04:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.331 4301560895441064192 296.92148688167 +09.07825934389 12.5115 12.1588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247049_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 247049_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 247052_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247052_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:07:04.07 +09:39:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.776 4299590849782512256 301.76753390389 +09.66057667893 11.6566 10.8542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247053_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247053_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:30:17.91 +08:39:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.079 4296306982201653248 292.57464559602 +08.66606342286 12.0933 11.5278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247054_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247054_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:00:40.69 +02:56:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 5.225 4241170532821013120 300.16954641091 +02.93754862566 11.4271 10.6821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247066_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247066_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:02:16.01 +04:58:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247067_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247067_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:32:58.48 +05:01:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247076_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247076_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:39:06.05 +05:24:39.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247083_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247083_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:04:13.64 +07:15:39.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247084_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247084_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:55:28.18 +06:24:03.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 247088_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247088_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:30:13.56 +02:52:44.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247096_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247096_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:25:21.26 +03:06:45.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 247098_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247098_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:55:31.74 +10:08:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247102_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247102_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:25:33.03 +03:05:11.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 247106_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247106_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:40:01.28 +07:32:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247108_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247108_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:22:49.05 +07:34:45.6 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 247109_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247109_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 247112_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247112_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:35:28.06 +09:11:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.687 4302176793749559936 293.86645456594 +09.19261473480 12.6775 12.1946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247115_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247115_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:25:34.40 +03:05:04.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 247117_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247117_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:28:27.07 +08:55:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.980 4296371784682912256 292.11291204781 +08.92301858700 12.5196 11.4654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247122_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247122_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:01:00.37 +09:51:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247129_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247129_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:27:52.73 +08:57:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247135_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247135_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:20:33.45 +09:45:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.091 4308637356595227904 290.13964910291 +09.75543080197 13.0781 12.4723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247138_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247138_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:37:42.07 +05:16:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.548 4291271154549036800 294.42585871202 +05.27638666860 13.3044 12.4778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247144_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247144_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:22:39.97 +07:32:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.978 4295708268100215552 290.66661363657 +07.53559406780 12.9892 12.3484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247148_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247148_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:32:06.10 +09:49:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247152_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247152_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:32:00.50 +08:04:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247162_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247162_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:48:25.48 +04:09:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247166_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247166_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:35:00.58 +09:23:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247168_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247168_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:55:55.73 +06:37:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247169_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247169_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:35:18.01 +07:15:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247174_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247174_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:53:24.51 +02:10:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247177_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247177_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:32:23.55 +09:35:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247187_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 247187_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:42:10.05 +07:09:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180789_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 180789_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:53:53.63 +09:39:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44257_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 44257_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:40:42.87 +03:12:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123775_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 123775_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:49:19.28 +06:51:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228472_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 228472_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:05:40.50 +09:14:45.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)
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Considering the candidate 70827_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 70827_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:51:29.64 +04:27:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32257_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 32257_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 228247_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 228247_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:05:51.58 +09:38:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90930_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 90930_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:40:15.43 +05:21:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165804_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 165804_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:57:29.12 +08:42:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127493_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 127493_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:54:28.66 +06:59:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73278_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 73278_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 113492_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 113492_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:48:18.30 +06:22:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125061_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 125061_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 27048_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 27048_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:16:16.03 +02:15:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32889_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 32889_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:28:31.23 +02:36:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196414_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 196414_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 46201_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 46201_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:59:42.51 +03:18:41.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 175254_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 175254_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:47:35.97 +09:56:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17141_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 17141_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 176545_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 176545_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:06:52.63 +09:51:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184320_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 184320_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 105185_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 105185_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:23:07.91 +05:55:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189590_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 189590_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:35:11.10 +09:09:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125952_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 125952_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:46:03.93 +06:55:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72237_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 72237_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:26:40.93 +04:26:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81425_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 81425_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:45:09.78 +04:54:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190573_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
Preparing report for the candidate 190573_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
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Considering the candidate 147875_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 147875_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:56:52.89 +07:54:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85186_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 85186_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 20:06:41.16 +05:09:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96747_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 96747_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:54:33.36 +05:40:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174553_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 174553_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
**** FOUND 19:40:43.09 +09:55:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116919_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041
The candidate 116919_fd_Aql-02-Q2b1x1_2026-04-02_04-16-51_20.00sec_-15.00C_LIGHT_0041 did not pass the final checks
