This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n
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
GDS_J1858566-030304,2461138.8475,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1858566-030304 20260408.3475 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4265578041745830272,2461138.8475,13.28,0.05,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
Gaia DR3 4265578041745830272 20260408.3475 13.28CV 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
Gaia DR3 4205939019193336448,2461138.8475,12.93,0.05,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 4205939019193336448 20260408.3475 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4253784886211996160,2461138.8475,12.89,0.05,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 4253784886211996160 20260408.3475 12.89CV 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
2MASS J18521087-0600097,2461138.8475,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J18521087-0600097 20260408.3475 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J19052982-0604579,2461138.8475,12.90,0.05,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
2MASS J19052982-0604579 20260408.3475 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FASTT 1326,2461138.8475,13.10,0.05,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
FASTT 1326 20260408.3475 13.10CV 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
NSVS J1844193-000013,2461138.8475,12.89,0.05,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
NSVS J1844193-000013 20260408.3475 12.89CV 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 11572,2461138.8475,12.69,0.05,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 11572 20260408.3475 12.69CV 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 J190552.27-004902.2,2461138.8475,12.64,0.05,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 J190552.27-004902.2 20260408.3475 12.64CV 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
NSVS 13980399,2461138.8475,12.50,0.05,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
NSVS 13980399 20260408.3475 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.8475,12.57,0.05,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
VARIABLE_NAME 20260408.3475 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
ASASSN-V J190727.87-055420.2,2461138.8475,12.68,0.05,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
ASASSN-V J190727.87-055420.2 20260408.3475 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
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
NSVS 13938866,2461138.8475,12.70,0.05,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
NSVS 13938866 20260408.3475 12.70CV 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
GDS_J1901216-013331,2461138.8475,13.02,0.05,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
GDS_J1901216-013331 20260408.3475 13.02CV 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 J190140-0212.0,2461138.8475,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190140-0212.0 20260408.3475 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
NSVS J1902406+021201,2461138.8475,12.57,0.05,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
NSVS J1902406+021201 20260408.3475 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
V1188 Aql,2461138.8475,11.11,0.05,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
V1188 Aql 20260408.3475 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
V1914 Aql,2461138.8475,11.58,0.05,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
V1914 Aql 20260408.3475 11.58CV 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 J190858.89-021344.0,2461138.8475,12.85,0.05,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
ASASSN-V J190858.89-021344.0 20260408.3475 12.85CV 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
ASAS J190428+0003.1,2461138.8475,12.46,0.05,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 J190428+0003.1 20260408.3475 12.46CV 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
NSVS 13966123,2461138.8475,12.62,0.05,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
NSVS 13966123 20260408.3475 12.62CV 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
V1513 Aql,2461138.8475,13.16,0.05,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
V1513 Aql 20260408.3475 13.16CV 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
V1553 Aql,2461138.8475,11.18,0.05,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
V1553 Aql 20260408.3475 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FASTT 1471,2461138.8475,12.84,0.05,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
FASTT 1471 20260408.3475 12.84CV 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
GDS_J1849154-042917,2461138.8475,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1849154-042917 20260408.3475 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1901138-003843,2461138.8475,13.08,0.05,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
GDS_J1901138-003843 20260408.3475 13.08CV 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
NSVS 13954052,2461138.8475,13.28,0.05,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
NSVS 13954052 20260408.3475 13.28CV 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
ASASSN-V J190340.80-043632.1,2461138.8475,12.25,0.05,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 J190340.80-043632.1 20260408.3475 12.25CV 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
NSVS 13982816,2461138.8475,11.71,0.05,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
NSVS 13982816 20260408.3475 11.71CV 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
NSVS 13963298,2461138.8475,12.04,0.05,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
NSVS 13963298 20260408.3475 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190748.38-060308.9,2461138.8475,12.86,0.05,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 J190748.38-060308.9 20260408.3475 12.86CV 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 J190837.46-054811.6,2461138.8475,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190837.46-054811.6 20260408.3475 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190503.92-044505.4,2461138.8475,12.71,0.05,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 J190503.92-044505.4 20260408.3475 12.71CV 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 J190713-0218.7,2461138.8475,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190713-0218.7 20260408.3475 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13984582,2461138.8475,12.35,0.05,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
NSVS 13984582 20260408.3475 12.35CV 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 J190522.48-013353.5,2461138.8475,12.52,0.05,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 J190522.48-013353.5 20260408.3475 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1831127-061441,2461138.8475,13.04,0.05,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
GDS_J1831127-061441 20260408.3475 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461138.84779934 08.04.2026 08:20:39.863 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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.: -8.06
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: 3 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): 8502
Objects passed selection criteria: 8486
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 7225.5
Average stars matched: 7026.5 (97.2459 %)
Memory usage VmPeak: 115536 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 03:23:11 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: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461138.84779934 08.04.2026 08:20:39.863 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 194
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 28 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): 102905
Objects passed selection criteria: 102631
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 81176.8
Average stars matched: 77666.5 (95.6758 %)
Memory usage VmPeak: 1948108 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 03:25:04 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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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: 2461138.84724168
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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits'
wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:12.868 -01:58:01.94
Angular distance between the image centers 0.0603 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:14.121 -01:58:37.29
Angular distance between the image centers 0.0511 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:12.868 -01:58:01.94
Second-epoch second image center 18:51:14.121 -01:58:37.29
Angular distance between the image centers 0.01112 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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.9yYYmF6opI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.UmIGk8Y5OJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits &> /tmp/tmp.EwH7p13TUX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits &> /tmp/tmp.4UrnA29JWj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat' -> 'wcsmag.cat'
Read 13310 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9619 to 290.7764 deg, Dec -7.2966 to +3.2981 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.9619 to 290.7764 deg, Dec -7.2966 to 3.2981 deg
Loaded 9541 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): 6890 out of 7408 total matches.
Matched with Tycho-2 7408 out of 13310 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.858998
a=0.000000 b=1.000000 c=22.858998
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
3.1 pix fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
3.0 pix fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Limiting magnitude estimates:
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
13.8 mag. fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
13.8 mag. fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.3 (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.9yYYmF6opI (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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1253, passed=13310
Got 13310 stars (including 12037 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 13310 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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.UmIGk8Y5OJ (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-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1265, passed=13307
Got 13307 stars (including 12019 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 13307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.EwH7p13TUX (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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=525, passed=6768
Got 6768 stars (including 6243 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 6768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.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.4UrnA29JWj (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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=507, passed=6788
Got 6788 stars (including 6277 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 6788 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20787_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 20787_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:47:01.91 -04:44:31.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11029_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 11029_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:02:20.93 +01:30:36.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:12.868 -01:58:01.94
Angular distance between the image centers 0.0603 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:14.121 -01:58:37.29
Angular distance between the image centers 0.0511 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:12.868 -01:58:01.94
Second-epoch second image center 18:51:14.121 -01:58:37.29
Angular distance between the image centers 0.01112 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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.9gj2kMEN77
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.kMHFa5jrGl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits &> /tmp/tmp.3PORI3BaEU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits &> /tmp/tmp.o1GpdKi1It
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat' -> 'wcsmag.cat'
Read 153764 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9569 to 290.7986 deg, Dec -7.2966 to +3.3005 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.9569 to 290.7986 deg, Dec -7.2966 to 3.3005 deg
Loaded 9554 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): 6421 out of 8387 total matches.
Matched with Tycho-2 8387 out of 153764 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.669636
a=0.000000 b=1.000000 c=22.669636
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 131 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.1 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
2.6 pix fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
2.6 pix fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Limiting magnitude estimates:
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
14.0 mag. fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
14.0 mag. fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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.9gj2kMEN77 (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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=17867, passed=153743
Got 153743 stars (including 135593 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 153743 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149678 with non-zero local correction accuracy
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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.kMHFa5jrGl (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-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=18180, passed=153307
Got 153307 stars (including 134827 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 153307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.3PORI3BaEU (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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=2, blended=5648, passed=58333
Got 58333 stars (including 52615 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 58333 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (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 413 to 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 57247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
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 413 to 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 57250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 57251 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.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.o1GpdKi1It (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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=1, blended=5731, passed=58900
Got 58900 stars (including 53114 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 58900 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 57825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 57828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 57828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-19-51_20.00sec_-4.90C_LIGHT_0169.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.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_2026-04-08_CI_Aql-03-Q2b1x1_032120_TTUQ2b1x1_15308_omsJx85n/wcs_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out164450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out164556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out26928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out81920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out126971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99382.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 20s
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Considering the candidate 177225_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 177225_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 177229_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 177229_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 177235_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177235_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:57:07.40 -04:19:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177237_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177237_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:03:03.97 -00:27:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 5.016 4265538631121224320 285.76544866393 -00.44980239673 11.5346 9.7948 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177238_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177238_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:26.30 +02:08:36.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 177241_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 177241_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 177251_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177251_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 177253_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177253_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:29.60 -01:55:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177257_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177257_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:03:33.20 -00:56:40.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 177261_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 177261_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 177266_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177266_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:03:07.58 -05:16:15.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177271_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177271_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:05.53 -00:54:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177273_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177273_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:43:12.15 -06:06:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177275_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177275_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:42:58.81 -04:32:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.190 4256720616564661504 280.74416666038 -04.54593455749 11.0438 9.5665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177276_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177276_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:05:34.94 -00:25:09.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177277_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177277_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:04:03.59 -05:08:52.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177317_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177317_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:47:01.88 -04:44:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177330_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177330_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:02:58.57 -03:43:12.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177342_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177342_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:43:01.50 -05:42:33.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177346_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177346_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:01:33.66 -05:43:10.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177371_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177371_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:37.24 +00:06:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177379_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177379_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:47:27.31 -05:43:52.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177392_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177392_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:56:59.89 -05:52:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177400_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177400_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:43.80 -02:25:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177417_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177417_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:04:34.33 -05:39:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177459_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177459_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:06:32.86 +01:16:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.790 4267494176915800320 286.63674083845 +01.27645182232 12.5836 11.2938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177465_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177465_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:05:31.52 -00:39:19.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177479_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177479_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:04.19 -03:51:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177487_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177487_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:48:28.56 -05:40:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.000 4253347108791216512 282.11876093555 -05.68125206701 11.5070 9.7728 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177488_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177488_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:54:59.18 -01:02:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.991 4265255605611296768 283.74548596109 -01.03486886011 11.5019 9.8805 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177490_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177490_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:29.01 -01:36:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.166 4262206561121136384 286.87202214709 -01.60284428076 12.3921 10.6483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177491_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177491_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:59:57.47 -04:38:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177492_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177492_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:06:26.57 -04:13:54.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177502_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177502_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:42.81 +00:35:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177504_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177504_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:04:48.96 -01:12:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177505_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177505_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:52:05.11 -05:12:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177515_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177515_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:05:21.19 -03:18:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.613 4260803206314668672 286.33900802584 -03.30937458478 11.4077 10.0372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177516_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177516_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:24:32.37 -01:32:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.739 4271261554734243072 276.13355809727 -01.53515435937 14.2610 12.2789 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177518_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177518_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:24:32.32 -03:31:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.739 4269640187389690624 276.13308317755 -03.52345784001 13.2905 11.2603 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177520_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177520_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:57:50.99 -01:59:00.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177521_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177521_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:05:04.45 +01:16:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.481 4267502938649052672 286.26920904384 +01.26761669559 13.4649 11.5378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177525_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 177525_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177535_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177535_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:59:12.24 +00:14:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177541_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177541_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:53:41.09 -05:03:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.924 4254931023988184192 283.42142902314 -05.06642072859 12.3225 10.8179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177546_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177546_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:53:19.32 -05:02:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.683 4254943217326300544 283.33047650642 -05.04541153760 11.6000 9.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177549_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177549_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:27:14.88 +00:53:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177559_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177559_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:01.09 -05:10:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177560_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177560_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:53:21.04 -04:21:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177570_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 177570_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:02:26.45 -04:58:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.066 4254335737151611392 285.61066903567 -04.97420542383 12.3535 10.8291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25904_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 25904_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 46681_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 46681_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:06:54.96 -05:03:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142751_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 142751_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115835_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 115835_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:53:57.41 +01:36:35.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132154_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 132154_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 164952_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 164952_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 32562_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 32562_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 165533_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 165533_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:56:26.37 -00:58:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.624 4265338313878640384 284.11037676627 -00.97647119540 10.6968 9.3051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 73075_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 73075_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:52:35.88 -03:12:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103890_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 103890_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:51:53.70 -00:58:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142804_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 142804_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 44410_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 44410_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:45:44.79 -05:14:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70668_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 70668_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:06:12.80 -03:24:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42147_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 42147_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 22456_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 22456_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:47:21.36 -06:16:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 2.885 4253248771225704064 281.83901658762 -06.27127353138 11.2820 9.6954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50838_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 50838_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 68736_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 68736_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:05:24.26 -03:35:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.112 4260741663691254912 286.35164225308 -03.59684829927 12.3385 10.3203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74720_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 74720_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:04:01.05 -03:05:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29776_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 29776_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 83700_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 83700_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:01:40.76 -02:21:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49595_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 49595_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 70335_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 70335_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:43:24.42 -03:30:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31780_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 31780_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:02:52.77 -05:50:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61778_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 61778_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:52.92 -04:05:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95332_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 95332_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:06:05.45 -01:29:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94632_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 94632_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 73022_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 73022_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:59:53.91 -03:14:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85292_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 85292_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 147796_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 147796_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 71757_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 71757_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:04:05.14 -03:20:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99382_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 99382_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 142326_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 142326_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:58:34.36 -00:47:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96276_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 96276_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:42:11.74 -01:28:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103039_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 103039_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:52:48.38 -01:01:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84634_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 84634_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:58:42.98 -02:16:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57707_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 57707_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 75227_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 75227_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:59.19 -03:01:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33038_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 33038_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:55:16.85 -05:47:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75955_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 75955_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:58:15.43 -03:00:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139263_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 139263_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:59:29.66 -00:34:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34502_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 34502_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:48:58.47 -05:44:02.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 31238_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 31238_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:34:21.24 -05:53:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85109_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 85109_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 146304_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 146304_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:53:14.20 +02:15:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41887_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 41887_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:40.00 -05:19:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94085_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 94085_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:08.66 -01:34:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131573_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 131573_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 30380_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 30380_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:51.33 -05:52:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165079_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 165079_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:08:07.13 -01:34:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92087_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 92087_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 73869_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 73869_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 164556_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 164556_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:40.16 -05:07:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.147 4206334529816172800 286.91820351650 -05.12230376590 12.6108 11.1681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 26928_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 26928_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:49:55.07 -06:04:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.071 4253272028378877312 282.47980498647 -06.07647479022 12.1288 10.5796 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 164450_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 164450_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:42:33.19 -04:35:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.982 4256714947207900416 280.63809804195 -04.59205372463 11.8028 10.1527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 126971_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 126971_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
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Considering the candidate 73000_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 73000_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:43:44.92 -03:16:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60096_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 60096_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:42:31.85 -04:17:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.212 4256741537311990528 280.63267606440 -04.28680853701 11.4113 9.7994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84001_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 84001_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:58:41.77 -02:20:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95394_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 95394_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167525_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 167525_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:41:07.24 -01:35:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.187 4259767466353941632 280.27984088658 -01.58619017614 11.1535 9.5444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87924_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 87924_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:01:58.42 -02:00:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39045_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 39045_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:33:07.23 -05:30:10.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98233_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 98233_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:59:11.38 -01:19:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146876_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 146876_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:02:20.92 +01:30:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28067_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 28067_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:07:38.65 -05:58:53.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56749_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 56749_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140512_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 140512_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66890_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 66890_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173105_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 173105_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:03:24.58 -00:32:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.568 4265533992516182912 285.85340048731 -00.54379647212 11.3881 9.7810 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31955_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 31955_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:09:12.27 -05:48:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54598_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 54598_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83576_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 83576_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39602_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 39602_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 18:48:41.08 -05:27:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41503_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 41503_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26510_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 26510_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31962_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 31962_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81920_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
The candidate 81920_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170 did not pass the final checks
**** FOUND 19:06:39.82 -02:28:05.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52238_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 52238_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83973_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 83973_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84941_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 84941_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94382_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 94382_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22997_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
Preparing report for the candidate 22997_fd_Aql-03-Q2b1x1_2026-04-08_03-20-39_20.00sec_-5.00C_LIGHT_0170
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 42s
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:02:56.63 +00:25:46.2
19:04:27.95 +00:03:05.1
18:44:18.91 -00:00:13.0
19:01:13.68 -00:38:45.7
19:00:59.66 -00:48:46.3
19:05:52.12 -00:49:03.6
19:02:39.96 +02:11:51.8
18:58:56.14 -03:03:03.9
19:02:08.89 -00:32:18.9
19:07:14.72 -06:04:08.7
18:56:37.94 -06:07:17.6
18:52:10.77 -06:00:03.0
18:31:13.11 -06:14:39.1
19:05:29.50 -06:04:54.7
19:07:48.15 -06:03:06.1
19:07:27.65 -05:54:16.7
19:08:37.11 -05:48:07.9
18:56:55.30 -05:48:54.1
18:56:04.63 -05:21:54.6
19:06:29.06 -05:18:51.2
18:37:12.90 -04:57:07.6
18:39:48.36 -04:52:45.2
19:05:03.73 -04:45:02.3
19:03:40.60 -04:36:31.7
18:49:15.56 -04:29:18.3
19:02:39.28 -04:19:10.7
18:49:23.26 -03:46:38.9
19:01:04.88 -03:10:47.8
19:08:00.25 -02:19:19.2
19:07:13.09 -02:18:46.3
19:09:06.59 -02:14:02.6
19:08:58.42 -02:13:44.6
19:01:40.32 -02:11:58.5
18:58:01.62 -01:43:51.7
19:05:22.25 -01:33:54.4
19:01:21.44 -01:33:33.7
19:01:42.58 -01:30:35.3
19:06:05.33 -01:12:16.5
########### Completed Aql-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:58:56.14 -03:03:03.9
19:02:08.89 -00:32:18.9
19:07:14.72 -06:04:08.7
18:56:37.94 -06:07:17.6
18:52:10.77 -06:00:03.0
19:05:29.50 -06:04:54.7
19:00:59.66 -00:48:46.3
18:44:18.91 -00:00:13.0
18:56:55.30 -05:48:54.1
19:05:52.12 -00:49:03.6
19:06:29.06 -05:18:51.2
18:39:48.36 -04:52:45.2
19:07:27.65 -05:54:16.7
18:37:12.90 -04:57:07.6
19:01:21.44 -01:33:33.7
19:01:40.32 -02:11:58.5
19:02:39.96 +02:11:51.8
19:06:05.33 -01:12:16.5
19:02:39.28 -04:19:10.7
19:08:58.42 -02:13:44.6
19:04:27.95 +00:03:05.1
18:58:01.62 -01:43:51.7
19:01:04.88 -03:10:47.8
19:02:56.63 +00:25:46.2
19:01:42.58 -01:30:35.3
18:49:15.56 -04:29:18.3
19:01:13.68 -00:38:45.7
18:49:23.26 -03:46:38.9
19:03:40.60 -04:36:31.7
19:08:00.25 -02:19:19.2
18:56:04.63 -05:21:54.6
19:07:48.15 -06:03:06.1
19:08:37.11 -05:48:07.9
19:05:03.73 -04:45:02.3
19:07:13.09 -02:18:46.3
19:09:06.59 -02:14:02.6
19:05:22.25 -01:33:54.4
18:31:13.11 -06:14:39.1
###################################################################################
18:58:56.14 -03:03:03.9 -- not an asteroid (will add it to exclusion list)
19:02:08.89 -00:32:18.9 -- not an asteroid (will add it to exclusion list)
19:07:14.72 -06:04:08.7 -- not an asteroid (will add it to exclusion list)
18:56:37.94 -06:07:17.6 -- not an asteroid (will add it to exclusion list)
18:52:10.77 -06:00:03.0 -- not an asteroid (will add it to exclusion list)
19:05:29.50 -06:04:54.7 -- not an asteroid (will add it to exclusion list)
19:00:59.66 -00:48:46.3 -- not an asteroid (will add it to exclusion list)
18:44:18.91 -00:00:13.0 -- not an asteroid (will add it to exclusion list)
18:56:55.30 -05:48:54.1 -- not an asteroid (will add it to exclusion list)
19:05:52.12 -00:49:03.6 -- not an asteroid (will add it to exclusion list)
19:06:29.06 -05:18:51.2 -- not an asteroid (will add it to exclusion list)
18:39:48.36 -04:52:45.2 -- not an asteroid (will add it to exclusion list)
19:07:27.65 -05:54:16.7 -- not an asteroid (will add it to exclusion list)
18:37:12.90 -04:57:07.6 -- not an asteroid (will add it to exclusion list)
19:01:21.44 -01:33:33.7 -- not an asteroid (will add it to exclusion list)
19:01:40.32 -02:11:58.5 -- not an asteroid (will add it to exclusion list)
19:02:39.96 +02:11:51.8 -- not an asteroid (will add it to exclusion list)
19:06:05.33 -01:12:16.5 -- not an asteroid (will add it to exclusion list)
19:02:39.28 -04:19:10.7 -- not an asteroid (will add it to exclusion list)
19:08:58.42 -02:13:44.6 -- not an asteroid (will add it to exclusion list)
19:04:27.95 +00:03:05.1 -- not an asteroid (will add it to exclusion list)
18:58:01.62 -01:43:51.7 -- not an asteroid (will add it to exclusion list)
19:01:04.88 -03:10:47.8 -- not an asteroid (will add it to exclusion list)
19:02:56.63 +00:25:46.2 -- not an asteroid (will add it to exclusion list)
19:01:42.58 -01:30:35.3 -- not an asteroid (will add it to exclusion list)
18:49:15.56 -04:29:18.3 -- not an asteroid (will add it to exclusion list)
19:01:13.68 -00:38:45.7 -- not an asteroid (will add it to exclusion list)
18:49:23.26 -03:46:38.9 -- not an asteroid (will add it to exclusion list)
19:03:40.60 -04:36:31.7 -- not an asteroid (will add it to exclusion list)
19:08:00.25 -02:19:19.2 -- not an asteroid (will add it to exclusion list)
18:56:04.63 -05:21:54.6 -- not an asteroid (will add it to exclusion list)
19:07:48.15 -06:03:06.1 -- not an asteroid (will add it to exclusion list)
19:08:37.11 -05:48:07.9 -- not an asteroid (will add it to exclusion list)
19:05:03.73 -04:45:02.3 -- not an asteroid (will add it to exclusion list)
19:07:13.09 -02:18:46.3 -- not an asteroid (will add it to exclusion list)
19:09:06.59 -02:14:02.6 -- not an asteroid (will add it to exclusion list)
19:05:22.25 -01:33:54.4 -- not an asteroid (will add it to exclusion list)
18:31:13.11 -06:14:39.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:31:13.11 -06:14:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:12.90 -04:57:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:39:48.36 -04:52:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:44:18.91 -00:00:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:15.56 -04:29:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:23.26 -03:46:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:10.77 -06:00:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:04.63 -05:21:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:37.94 -06:07:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:55.30 -05:48:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:01.62 -01:43:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:56.14 -03:03:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:59.66 -00:48:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:04.88 -03:10:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:13.68 -00:38:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:21.44 -01:33:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:40.32 -02:11:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:42.58 -01:30:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:08.89 -00:32:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:39.28 -04:19:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:39.96 +02:11:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:56.63 +00:25:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:40.60 -04:36:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:27.95 +00:03:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:03.73 -04:45:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:22.25 -01:33:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:29.50 -06:04:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:52.12 -00:49:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:05.33 -01:12:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:29.06 -05:18:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:13.09 -02:18:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:14.72 -06:04:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:27.65 -05:54:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:48.15 -06:03:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:00.25 -02:19:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:37.11 -05:48:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:58.42 -02:13:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:06.59 -02:14:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
18:31:13.11 -06:14:39.1 -- a known variable star
18:37:12.90 -04:57:07.6 -- a known variable star
18:39:48.36 -04:52:45.2 -- a known variable star
18:44:18.91 -00:00:13.0 -- a known variable star
18:49:15.56 -04:29:18.3 -- a known variable star
18:49:23.26 -03:46:38.9 -- a known variable star
18:52:10.77 -06:00:03.0 -- a known variable star
18:56:04.63 -05:21:54.6 -- a known variable star
18:56:37.94 -06:07:17.6 -- not a known variable star
18:56:55.30 -05:48:54.1 -- a known variable star
18:58:01.62 -01:43:51.7 -- a known variable star
18:58:56.14 -03:03:03.9 -- a known variable star
19:00:59.66 -00:48:46.3 -- a known variable star
19:01:04.88 -03:10:47.8 -- a known variable star
19:01:13.68 -00:38:45.7 -- a known variable star
19:01:21.44 -01:33:33.7 -- a known variable star
19:01:40.32 -02:11:58.5 -- a known variable star
19:01:42.58 -01:30:35.3 -- a known variable star
19:02:08.89 -00:32:18.9 -- a known variable star
19:02:39.28 -04:19:10.7 -- a known variable star
19:02:39.96 +02:11:51.8 -- a known variable star
19:02:56.63 +00:25:46.2 -- a known variable star
19:03:40.60 -04:36:31.7 -- a known variable star
19:04:27.95 +00:03:05.1 -- a known variable star
19:05:03.73 -04:45:02.3 -- a known variable star
19:05:22.25 -01:33:54.4 -- a known variable star
19:05:29.50 -06:04:54.7 -- a known variable star
19:05:52.12 -00:49:03.6 -- a known variable star
19:06:05.33 -01:12:16.5 -- a known variable star
19:06:29.06 -05:18:51.2 -- a known variable star
19:07:13.09 -02:18:46.3 -- a known variable star
19:07:14.72 -06:04:08.7 -- not a known variable star
19:07:27.65 -05:54:16.7 -- a known variable star
19:07:48.15 -06:03:06.1 -- a known variable star
19:08:00.25 -02:19:19.2 -- a known variable star
19:08:37.11 -05:48:07.9 -- a known variable star
19:08:58.42 -02:13:44.6 -- a known variable star
19:09:06.59 -02:14:02.6 -- a known variable star
Found 2 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
38 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
18:31:13.11 -06:14:39.1
18:37:12.90 -04:57:07.6
18:39:48.36 -04:52:45.2
18:44:18.91 -00:00:13.0
18:49:15.56 -04:29:18.3
18:49:23.26 -03:46:38.9
18:52:10.77 -06:00:03.0
18:56:04.63 -05:21:54.6
18:56:37.94 -06:07:17.6
18:56:55.30 -05:48:54.1
18:58:01.62 -01:43:51.7
18:58:56.14 -03:03:03.9
19:00:59.66 -00:48:46.3
19:01:04.88 -03:10:47.8
19:01:13.68 -00:38:45.7
19:01:21.44 -01:33:33.7
19:01:40.32 -02:11:58.5
19:01:42.58 -01:30:35.3
19:02:08.89 -00:32:18.9
19:02:39.28 -04:19:10.7
19:02:39.96 +02:11:51.8
19:02:56.63 +00:25:46.2
19:03:40.60 -04:36:31.7
19:04:27.95 +00:03:05.1
19:05:03.73 -04:45:02.3
19:05:22.25 -01:33:54.4
19:05:29.50 -06:04:54.7
19:05:52.12 -00:49:03.6
19:06:05.33 -01:12:16.5
19:06:29.06 -05:18:51.2
19:07:13.09 -02:18:46.3
19:07:14.72 -06:04:08.7
19:07:27.65 -05:54:16.7
19:07:48.15 -06:03:06.1
19:08:00.25 -02:19:19.2
19:08:37.11 -05:48:07.9
19:08:58.42 -02:13:44.6
19:09:06.59 -02:14:02.6
18:42:33.19 -04:35:30.7
19:07:40.16 -05:07:20.7
18:56:26.37 -00:58:37.2
18:41:07.24 -01:35:10.1
19:03:24.58 -00:32:38.1
19:03:03.97 -00:27:02.4
19:08:26.30 +02:08:36.6
19:03:33.20 -00:56:40.9
19:03:07.58 -05:16:15.3
18:42:58.81 -04:32:44.8
19:05:34.94 -00:25:09.1
19:04:03.59 -05:08:52.9
19:06:32.86 +01:16:35.7
18:48:28.56 -05:40:50.7
18:54:59.18 -01:02:06.1
19:07:29.01 -01:36:10.8
19:05:21.19 -03:18:33.3
18:24:32.37 -01:32:06.5
18:24:32.32 -03:31:25.2
19:05:04.45 +01:16:00.9
18:53:41.09 -05:03:56.3
18:53:19.32 -05:02:40.8
19:02:26.45 -04:58:25.9
18:47:21.36 -06:16:13.7
18:49:55.07 -06:04:32.5
18:48:58.47 -05:44:02.4
18:42:31.85 -04:17:08.3
19:05:24.26 -03:35:48.0
19:06:39.82 -02:28:05.2
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461138.84724168 -observatory V36
23:29:47.31 -05:39:31.7 Mercury (0.3mag)
02:31:43.29 +14:46:60.0 Venus (-3.9mag)
23:56:03.74 -01:32:02.3 Mars (1.2mag)
07:09:28.32 +22:51:15.7 Jupiter (-2.2mag)
00:25:44.41 +00:27:24.1 Saturn (0.9mag)
03:46:08.38 +19:42:26.9 Uranus (5.8mag)
00:09:49.33 -00:21:48.8 Neptune (7.8mag)
20:33:21.94 -22:52:27.3 Pluto (14.5mag)
17:52:39.00 -28:55:39.0 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Apr 8 03:23 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461138.84724168:
07:09:22.32 +22:51:25.5 Io (5.7mag)
07:09:19.92 +22:51:35.0 Europa (5.9mag)
07:09:48.73 +22:50:34.4 Ganymede (5.3mag)
07:08:53.63 +22:52:25.2 Callisto (6.5mag)
07:13:06.91 +22:42:38.3 Himalia (15.3mag)
07:09:30.27 +22:51:13.7 Thebe (16.2mag)
07:13:07.75 +23:11:51.0 Elara (17.3mag)
07:07:49.95 +23:35:16.2 Pasiphae (17.4mag)
07:17:57.66 +22:48:27.5 Carme (18.4mag)
00:25:47.81 +00:27:14.3 Titan (8.8mag)
00:25:49.87 +00:27:24.9 Rhea (10.1mag)
00:25:40.05 +00:28:41.9 Iapetus (11.5mag)
00:25:53.52 +00:27:09.6 Hyperion (14.8mag)
00:27:27.12 +00:37:00.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 03:23 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461138.84724168:
14:59:13.17 -10:16:45.2 JWST
14:42:15.01 +55:58:20.5 Chandra
08:30:15.96 -46:45:47.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 03:23 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461138.84724168 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:21.10 -28:20:58.6 13.9mag P/2010 H2 (Vales)
05:01:28.42 -70:02:13.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:56.19 +31:23:18.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:54.99 +09:37:52.7 17.6mag C/2021 G2 (ATLAS)
23:08:01.85 +28:56:30.9 17.0mag C/2022 E2 (ATLAS)
04:20:25.68 +25:49:32.6 15.9mag C/2022 N2 (PANSTARRS)
09:02:06.29 +31:56:27.3 16.2mag C/2022 QE78 (ATLAS)
08:30:08.84 -00:59:17.1 17.3mag C/2022 R6 (PANSTARRS)
18:55:16.01 +17:52:52.0 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:57.15 -11:37:52.4 17.6mag P/2023 B1 (PANSTARRS)
09:11:34.22 -13:08:19.4 17.6mag C/2023 F3 (ATLAS)
21:46:00.00 +62:28:53.5 17.5mag C/2023 H5 (Lemmon)
19:25:03.01 -03:37:46.6 14.2mag C/2023 R1 (PANSTARRS)
21:41:48.30 +84:53:03.3 17.8mag C/2023 X2 (Lemmon)
06:15:02.47 +63:33:47.4 17.1mag C/2024 A1 (ATLAS)
04:56:10.89 +15:28:36.3 10.5mag C/2024 E1 (Wierzchos)
16:23:54.78 +05:07:56.5 17.4mag C/2024 G6 (ATLAS)
20:18:21.50 +13:14:21.5 14.7mag C/2024 J3 (ATLAS)
03:19:37.07 -23:34:36.8 16.4mag C/2024 T5 (ATLAS)
05:10:24.12 +47:15:16.6 17.7mag C/2025 J1 (Borisov)
14:10:27.53 +39:28:54.7 14.9mag C/2025 L1 (ATLAS)
03:13:32.19 -25:03:30.3 17.8mag C/2025 Q3 (ATLAS)
22:59:54.45 +19:48:22.2 9.7mag C/2025 R3 (PANSTARRS)
12:57:27.09 +02:31:57.2 17.5mag C/2025 Y1 (ATLAS)
02:05:55.40 +03:57:08.2 9.7mag C/2026 A1 (MAPS)
23:37:18.62 +35:42:39.5 14.3mag C/2026 B2 (Sun-Gao)
18:28:00.41 -10:06:53.3 12.3mag 10P/Tempel
15:10:17.87 +03:56:06.5 13.3mag 24P/Schaumasse
11:05:03.37 -01:47:09.6 15.7mag 29P/Schwassmann-Wachmann
17:57:56.13 -09:54:20.9 17.8mag 40P/Vaisala
10:38:25.32 -04:44:57.6 16.8mag 43P/Wolf-Harrington
01:36:51.87 +16:10:17.2 17.2mag 47P/Ashbrook-Jackson
06:57:01.69 +38:37:58.4 17.0mag 63P/Wild
23:19:09.37 -12:23:08.7 15.7mag 65P/Gunn
03:43:10.77 +18:32:13.9 15.9mag 76P/West-Kohoutek-Ikemura
00:48:46.14 +06:42:53.4 14.4mag 78P/Gehrels
22:39:23.13 -11:38:39.5 14.5mag 88P/Howell
01:49:03.45 +18:33:12.9 15.1mag 93P/Lovas
04:40:44.27 +31:51:26.3 16.3mag 123P/West-Hartley
08:19:59.80 +41:53:41.2 16.2mag 124P/Mrkos
02:21:29.01 +13:30:17.7 16.4mag 128P/Shoemaker-Holt
02:32:35.11 +13:32:02.1 17.5mag 131P/Mueller
00:46:40.96 +10:26:44.0 11.1mag 141P/Machholz
00:56:29.50 +02:00:04.7 11.1mag 141P-A/Machholz
23:45:48.54 -01:44:34.3 13.8mag 141P-D/Machholz
01:25:56.87 +03:41:56.8 17.9mag 141P-I/Machholz
00:41:06.46 -05:21:08.6 15.2mag 162P/SidingSpring
10:30:19.15 +31:22:25.8 17.9mag 164P/Christensen
06:22:22.66 +24:28:13.8 17.9mag 198P/ODAS
15:04:58.09 -00:55:42.5 17.4mag 210P/Christensen
21:15:47.25 -13:18:03.2 17.5mag 218P/LINEAR
17:13:45.00 -14:49:52.7 16.2mag 235P/LINEAR
05:18:09.80 +34:03:34.4 16.6mag 240P/NEAT
07:35:02.51 -06:01:48.7 17.6mag 242P/Spahr
15:45:18.98 +06:27:52.5 17.5mag 391P/Kowalski
07:31:32.65 +21:19:40.9 17.6mag 450P/LONEOS
05:24:54.78 +45:28:57.7 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 03:23 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 8 03:23 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 8 03:23 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:46:09.818 -61:19:51.60 AT 2026icy 2026-04-02.36 18.325
15:30:09.406 +58:57:13.42 AT 2026icx 2026-03-30.43 19.684
11:28:54.874 +21:06:30.69 AT 2026icw 2026-04-02.30 19.2031
12:10:50.697 +66:55:30.99 SN 2026icv 2026-04-02.28 18.5118
07:36:32.513 +50:19:24.81 AT 2026icu 2026-04-02.24 19.2237
08:38:37.560 +02:03:38.03 AT 2026ict 2026-04-02.15 19.0837
10:11:03.633 -05:31:15.36 AT 2026ics 2026-04-02.23 18.6573
11:09:42.183 +10:32:49.70 AT 2026icr 2026-03-24.33 20.476
10:16:29.552 -18:01:01.61 AT 2026icq 2026-03-25.18 20.2716
18:12:46.220 -18:40:42.30 AT 2026icp 2026-04-02.23 18.9
07:46:30.650 +27:23:24.16 AT 2026ico 2026-03-30.16 19.803
07:04:53.063 +10:28:54.71 AT 2026icn 2026-03-29.17 19.8144
10:09:06.230 +29:30:55.76 AT 2026icm 2026-03-27.16 20.1135
08:07:47.384 -00:23:25.65 AT 2026icl 2026-03-30.25 19.1418
07:33:52.396 +16:18:53.23 AT 2026ick 2026-03-30.19 19.5464
03:49:33.049 -49:30:53.67 AT 2026icj 2026-02-23.11 23.84
15:40:04.940 -18:30:53.00 AT 2026ici 2026-03-29.36 18.4
16:52:58.870 -62:16:14.10 AT 2026ich 2026-04-01.35 16.9
19:13:48.516 +60:10:55.03 AT 2026icg 2026-03-28.56 18.844
07:51:19.796 +21:17:20.06 AT 2026icf 2026-03-30.91 18.372
-rw-r--r-- 1 apache apache 30K Apr 8 03:23 tns_transients_list.txt
