This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ
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
FASTT 1179,2461132.8705,10.76,0.05,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 1179 20260402.3705 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.3753-01.1771,2461132.8705,12.69,0.05,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
ATO J288.3753-01.1771 20260402.3705 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
ATO J286.6566+00.0958,2461132.8705,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6566+00.0958 20260402.3705 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J287.7535+00.5210,2461132.8705,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.7535+00.5210 20260402.3705 12.72CV 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 4267887325388340736,2461132.8705,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267887325388340736 20260402.3705 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267887325388340736,2461132.8705,12.53,0.05,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 4267887325388340736 20260402.3705 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J287.0692-04.1986,2461132.8705,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0692-04.1986 20260402.3705 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.5051-06.0931,2461132.8705,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.5051-06.0931 20260402.3705 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267943293061106176,2461132.8705,11.41,0.05,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 4267943293061106176 20260402.3705 11.41CV 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
V1708 Aql,2461132.8705,12.04,0.05,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
V1708 Aql 20260402.3705 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
NSVS J1833072-053012,2461132.8705,12.47,0.05,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 J1833072-053012 20260402.3705 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1907520-055242,2461132.8705,12.71,0.05,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
NSVS J1907520-055242 20260402.3705 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
GDS_J1901408-022100,2461132.8705,12.55,0.05,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_J1901408-022100 20260402.3705 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1526 Aql,2461132.8705,12.42,0.05,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
V1526 Aql 20260402.3705 12.42CV 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
V1507 Aql,2461132.8705,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1507 Aql 20260402.3705 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4264705300032091136,2461132.8705,12.63,0.05,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 4264705300032091136 20260402.3705 12.63CV 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 4261069867919134464,2461132.8705,12.63,0.05,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 4261069867919134464 20260402.3705 12.63CV 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 J18524849-0101222,2461132.8705,12.64,0.05,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
2MASS J18524849-0101222 20260402.3705 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
GDS_J1859298-003424,2461132.8705,12.34,0.05,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_J1859298-003424 20260402.3705 12.34CV 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 J1908531-040554,2461132.8705,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1908531-040554 20260402.3705 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1904055-032040,2461132.8705,12.62,0.05,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 J1904055-032040 20260402.3705 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
NSVS 13982307,2461132.8705,12.82,0.05,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 13982307 20260402.3705 12.82CV 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
V1520 Aql,2461132.8705,11.06,0.05,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
V1520 Aql 20260402.3705 11.06CV 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 J191310-0154.7,2461132.8705,11.04,0.05,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
ASAS J191310-0154.7 20260402.3705 11.04CV 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
ZTF J190909.55+011727.4,2461132.8705,12.47,0.05,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
ZTF J190909.55+011727.4 20260402.3705 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191309.67-031351.2,2461132.8705,12.35,0.05,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
ASASSN-V J191309.67-031351.2 20260402.3705 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
2MASS J19094206-0004160,2461132.8705,12.63,0.05,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 J19094206-0004160 20260402.3705 12.63CV 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 1190,2461132.8705,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FASTT 1190 20260402.3705 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4253403974080315392,2461132.8705,12.11,0.05,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
Gaia DR3 4253403974080315392 20260402.3705 12.11CV 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
Gaia DR3 4253206336979410560,2461132.8705,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4253206336979410560 20260402.3705 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 4256222194201231488,2461132.8705,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4256222194201231488 20260402.3705 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191045.77-031846.6,2461132.8705,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191045.77-031846.6 20260402.3705 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0966 Aql,2461132.8705,11.27,0.05,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
V0966 Aql 20260402.3705 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1196 Aql,2461132.8705,11.96,0.05,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
V1196 Aql 20260402.3705 11.96CV 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
NSVS 13981119,2461132.8705,11.91,0.05,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 13981119 20260402.3705 11.91CV 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 13980035,2461132.8705,12.56,0.05,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 13980035 20260402.3705 12.56CV 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 J191204.01+005345.7,2461132.8705,12.47,0.05,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 J191204.01+005345.7 20260402.3705 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461132.87085800 02.04.2026 08:53:52.131 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9791
Objects passed selection criteria: 9763
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: 7546.5
Average stars matched: 7320 (96.9986 %)
Memory usage VmPeak: 117232 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:06:51 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: 2461132.87085800 02.04.2026 08:53:52.131 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 195
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: 26 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): 115218
Objects passed selection criteria: 114926
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 84773.8
Average stars matched: 80908.5 (95.4405 %)
Memory usage VmPeak: 1955696 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:09:38 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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461132.87010387
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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits'
wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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 18:51:44.705 -01:59:58.12
Angular distance between the image centers 0.08 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 18:51:47.832 -02:00:41.51
Angular distance between the image centers 0.10 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 18:51:44.705 -01:59:58.12
Second-epoch second image center 18:51:47.832 -02:00:41.51
Angular distance between the image centers 0.01774 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.tVz3MwASWV
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.8BYtaklkKd
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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits &> /tmp/tmp.TKPnNhQlY4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.N1Wjilp4lA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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 1 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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
3.1 pix fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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
13.7 mag. fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
13.7 mag. fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tVz3MwASWV (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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
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
Estimated accuracy of the plate solution: 0.37"
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.8BYtaklkKd (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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
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
Estimated accuracy of the plate solution: 0.37"
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.TKPnNhQlY4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=418, passed=5135
Got 5135 stars (including 4712 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 5135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.83"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.93"
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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.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.N1Wjilp4lA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=414, passed=5196
Got 5196 stars (including 4780 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 5196 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 -7.4 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...
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.83"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 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
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.93"
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_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out11029.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11029_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 11029_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
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 ####
19:02:20.98 +01:30:36.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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 18:51:44.705 -01:59:58.12
Angular distance between the image centers 0.08 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 18:51:47.832 -02:00:41.51
Angular distance between the image centers 0.10 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 18:51:44.705 -01:59:58.12
Second-epoch second image center 18:51:47.832 -02:00:41.51
Angular distance between the image centers 0.01774 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.LJiXOXhRWK
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.NmeiA5so5F
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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits &> /tmp/tmp.CTXnPpobeZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.RLimA18nxO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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 107 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
2.7 pix fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
2.6 pix fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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
13.7 mag. fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
13.7 mag. fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LJiXOXhRWK (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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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
Estimated accuracy of the plate solution: 0.40"
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.NmeiA5so5F (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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
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
Estimated accuracy of the plate solution: 0.43"
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.CTXnPpobeZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=3528, passed=44588
Got 44588 stars (including 40997 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 44588 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.88"
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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.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.RLimA18nxO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3662, passed=45320
Got 45320 stars (including 41608 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 45320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.77"
Estimated accuracy of the plate solution: 0.86"
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_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/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_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-52-46_20.00sec_-14.90C_LIGHT_0020.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Aql-03-Q2b1x1_040256_TTUQ2b1x1_22477_0TNy80CZ/wcs_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out164531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out45130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out103039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95332.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 30s
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: 17s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178600_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178600_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:56:54.43 -03:07:03.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178601_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178601_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:10:24.71 -03:09:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.603 4260679816165305344 287.60404412308 -03.16259453923 12.3706 10.9218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178603_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178603_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:09:23.03 +00:47:09.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178605_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178605_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178610_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178610_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178612_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178612_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:04:27.97 +00:12:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178616_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178616_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178618_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178618_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:12:41.65 +02:10:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.619 4267860005052446848 288.17459741745 +02.18056693426 12.4174 11.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178623_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178623_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:43:12.14 -06:06:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178624_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178624_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:11:05.06 +01:19:25.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178625_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178625_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178629_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178629_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178631_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178631_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:39:44.42 -03:49:15.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178635_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178635_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:09:17.34 -01:41:11.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178638_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178638_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:15:24.96 -03:28:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 4.215 4212947031420348672 288.85318741882 -03.46923308573 11.6535 11.0840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178639_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178639_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:14:02.68 -03:17:27.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178641_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178641_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:01:37.99 -03:33:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.729 4255527401598493056 285.40806741849 -03.55405345600 12.4085 11.3858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178642_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178642_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:10:10.49 +01:04:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 3.900 4267334713373582976 287.54477914554 +01.07855735484 12.0061 10.5645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178649_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178649_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178650_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178650_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178652_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178652_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:13:56.26 +02:13:01.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178653_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178653_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:03:31.90 -05:44:32.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178659_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178659_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178666_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 178666_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178721_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178721_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:47:01.86 -04:44:31.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178731_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178731_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:02:58.70 -03:43:12.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178737_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178737_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:57:03.65 -05:49:05.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178750_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178750_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:01:33.59 -05:43:08.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178790_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178790_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:05:13.34 +01:52:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178813_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178813_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:07:37.19 +00:06:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178817_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178817_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:57:32.22 -06:14:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178823_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178823_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:56:59.73 -05:53:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178843_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178843_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:45:04.02 -05:29:21.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178874_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178874_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:07:43.95 -02:25:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178879_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178879_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:56:56.84 -00:47:05.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178898_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178898_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:10:41.58 +00:15:28.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178908_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178908_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:09:27.30 -00:50:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178958_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 178958_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:08:04.26 -03:50:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45130_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 45130_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:04:04.79 -05:09:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 5.725 4254371991005594240 286.02069180770 -05.15630135598 10.8485 9.4175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115835_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 115835_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39045_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 39045_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31238_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 31238_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:34:21.18 -05:53:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164531_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 164531_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:54:34.92 -00:35:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.430 4265422147262975104 283.64628172938 -00.58384407162 11.5763 10.0832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30380_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 30380_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83983_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 83983_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:42:23.71 -02:22:02.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75955_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 75955_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:58:15.47 -03:00:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65381_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 65381_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:13:47.76 -03:49:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33038_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 33038_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:55:16.84 -05:47:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83700_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 83700_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103890_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 103890_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:51:53.75 -00:58:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95332_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 95332_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73022_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 73022_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96085_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 96085_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:10:10.68 -01:26:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116069_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 116069_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77497_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 77497_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103039_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 103039_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84634_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 84634_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:58:43.00 -02:16:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35089_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 35089_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:43:01.55 -05:42:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139263_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 139263_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31780_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 31780_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:02:52.82 -05:50:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61778_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 61778_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73075_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 73075_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:52:35.91 -03:12:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77479_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 77479_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:14:58.01 -02:49:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165675_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 165675_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:15:55.98 -02:17:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71757_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 71757_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73000_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 73000_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:43:44.84 -03:16:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.851 4258599230929763328 280.93604561870 -03.26992712049 11.3294 9.6291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165527_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 165527_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:05:41.79 -06:10:44.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98233_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 98233_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:59:11.43 -01:19:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41887_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 41887_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165168_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 165168_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:08:07.14 -01:34:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165162_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 165162_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:09:00.95 +00:21:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35000_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 35000_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:06:36.75 -05:39:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.269 4206244271105929344 286.65405034202 -05.66391389372 11.4400 9.8190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87924_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 87924_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146876_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 146876_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:02:20.95 +01:30:36.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142326_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 142326_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:58:34.39 -00:47:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146304_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 146304_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:53:14.21 +02:15:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88792_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 88792_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96276_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 96276_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:42:11.66 -01:28:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31955_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 31955_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:09:12.31 -05:48:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100368_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 100368_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:14:44.90 -01:08:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146622_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 146622_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72685_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 72685_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75227_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 75227_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:08:59.24 -03:01:46.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51284_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 51284_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:24:41.60 -04:51:17.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86878_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 86878_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:11:31.58 -02:05:24.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84001_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 84001_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:58:41.81 -02:20:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22698_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 22698_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (33.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28067_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 28067_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:07:38.59 -05:58:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147949_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 147949_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:13:24.75 +01:18:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133285_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 133285_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73992_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 73992_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:10:58.56 -03:08:39.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125608_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 125608_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39602_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 39602_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:48:41.11 -05:27:56.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23552_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 23552_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22207_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 22207_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151452_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 151452_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:13:38.90 +01:20:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26216_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 26216_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70335_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 70335_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:43:24.39 -03:30:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71929_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 71929_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87474_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 87474_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74720_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 74720_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:04:01.11 -03:05:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135709_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 135709_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46681_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 46681_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44410_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 44410_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 18:45:44.76 -05:14:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166636_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
The candidate 166636_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021 did not pass the final checks
**** FOUND 19:15:59.18 -01:47:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70668_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 70668_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121379_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
Preparing report for the candidate 121379_fd_Aql-03-Q2b1x1_2026-04-02_03-53-52_20.00sec_-15.00C_LIGHT_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 49s
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 ####
19:02:20.98 +01:30:36.8
18:52:48.44 -01:01:23.3
18:53:57.46 +01:36:35.6
19:14:42.64 +01:07:53.1
19:12:03.25 +00:53:40.6
18:52:21.80 +00:32:25.0
19:09:41.86 -00:04:17.3
19:14:45.82 -00:16:58.5
18:59:29.67 -00:34:25.3
19:09:09.23 +01:17:24.1
19:13:31.22 -01:10:47.7
19:06:38.04 +00:06:02.9
19:11:00.27 +00:31:22.0
19:15:08.58 +02:06:11.5
19:15:07.77 +02:06:07.8
19:08:15.71 -04:11:58.8
19:05:59.22 -06:04:49.3
19:14:23.01 +02:20:52.7
18:45:34.41 -06:17:18.8
18:43:36.09 -06:14:02.5
18:32:44.69 -06:06:38.8
19:07:51.38 -05:52:36.6
18:33:07.24 -05:30:10.5
19:07:39.98 -05:19:37.5
19:06:55.02 -05:03:21.9
19:08:52.95 -04:05:48.7
19:06:12.84 -03:24:38.2
19:04:05.26 -03:20:39.2
19:10:45.42 -03:18:46.9
19:13:09.24 -03:13:52.1
18:59:53.88 -03:14:30.4
19:11:22.06 -02:50:25.5
19:01:40.79 -02:21:00.7
19:11:59.63 -02:02:08.1
19:01:58.44 -02:00:47.5
19:13:10.30 -01:54:44.3
19:06:05.60 -01:30:00.0
########### 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 ####
19:02:20.98 +01:30:36.8
19:13:31.22 -01:10:47.7
19:06:38.04 +00:06:02.9
19:11:00.27 +00:31:22.0
19:15:08.58 +02:06:11.5
19:15:07.77 +02:06:07.8
19:08:15.71 -04:11:58.8
19:05:59.22 -06:04:49.3
19:14:23.01 +02:20:52.7
18:53:57.46 +01:36:35.6
18:33:07.24 -05:30:10.5
19:07:51.38 -05:52:36.6
19:01:40.79 -02:21:00.7
19:06:05.60 -01:30:00.0
18:59:53.88 -03:14:30.4
19:14:42.64 +01:07:53.1
19:11:22.06 -02:50:25.5
18:52:48.44 -01:01:23.3
18:59:29.67 -00:34:25.3
19:08:52.95 -04:05:48.7
19:04:05.26 -03:20:39.2
19:07:39.98 -05:19:37.5
19:01:58.44 -02:00:47.5
19:13:10.30 -01:54:44.3
19:09:09.23 +01:17:24.1
19:13:09.24 -03:13:52.1
19:09:41.86 -00:04:17.3
18:52:21.80 +00:32:25.0
18:43:36.09 -06:14:02.5
18:45:34.41 -06:17:18.8
18:32:44.69 -06:06:38.8
19:10:45.42 -03:18:46.9
19:11:59.63 -02:02:08.1
19:14:45.82 -00:16:58.5
19:06:55.02 -05:03:21.9
19:06:12.84 -03:24:38.2
19:12:03.25 +00:53:40.6
###################################################################################
19:02:20.98 +01:30:36.8 -- not an asteroid (will add it to exclusion list)
19:13:31.22 -01:10:47.7 -- not an asteroid (will add it to exclusion list)
19:06:38.04 +00:06:02.9 -- not an asteroid (will add it to exclusion list)
19:11:00.27 +00:31:22.0 -- not an asteroid (will add it to exclusion list)
19:15:08.58 +02:06:11.5 -- not an asteroid (will add it to exclusion list)
19:15:07.77 +02:06:07.8 -- not an asteroid (will add it to exclusion list)
19:08:15.71 -04:11:58.8 -- not an asteroid (will add it to exclusion list)
19:05:59.22 -06:04:49.3 -- not an asteroid (will add it to exclusion list)
19:14:23.01 +02:20:52.7 -- not an asteroid (will add it to exclusion list)
18:53:57.46 +01:36:35.6 -- not an asteroid (will add it to exclusion list)
18:33:07.24 -05:30:10.5 -- not an asteroid (will add it to exclusion list)
19:07:51.38 -05:52:36.6 -- not an asteroid (will add it to exclusion list)
19:01:40.79 -02:21:00.7 -- not an asteroid (will add it to exclusion list)
19:06:05.60 -01:30:00.0 -- not an asteroid (will add it to exclusion list)
18:59:53.88 -03:14:30.4 -- not an asteroid (will add it to exclusion list)
19:14:42.64 +01:07:53.1 -- not an asteroid (will add it to exclusion list)
19:11:22.06 -02:50:25.5 -- not an asteroid (will add it to exclusion list)
18:52:48.44 -01:01:23.3 -- not an asteroid (will add it to exclusion list)
18:59:29.67 -00:34:25.3 -- not an asteroid (will add it to exclusion list)
19:08:52.95 -04:05:48.7 -- not an asteroid (will add it to exclusion list)
19:04:05.26 -03:20:39.2 -- not an asteroid (will add it to exclusion list)
19:07:39.98 -05:19:37.5 -- not an asteroid (will add it to exclusion list)
19:01:58.44 -02:00:47.5 -- not an asteroid (will add it to exclusion list)
19:13:10.30 -01:54:44.3 -- not an asteroid (will add it to exclusion list)
19:09:09.23 +01:17:24.1 -- not an asteroid (will add it to exclusion list)
19:13:09.24 -03:13:52.1 -- not an asteroid (will add it to exclusion list)
19:09:41.86 -00:04:17.3 -- not an asteroid (will add it to exclusion list)
18:52:21.80 +00:32:25.0 -- not an asteroid (will add it to exclusion list)
18:43:36.09 -06:14:02.5 -- not an asteroid (will add it to exclusion list)
18:45:34.41 -06:17:18.8 -- not an asteroid (will add it to exclusion list)
18:32:44.69 -06:06:38.8 -- not an asteroid (will add it to exclusion list)
19:10:45.42 -03:18:46.9 -- not an asteroid (will add it to exclusion list)
19:11:59.63 -02:02:08.1 -- not an asteroid (will add it to exclusion list)
19:14:45.82 -00:16:58.5 -- not an asteroid (will add it to exclusion list)
19:06:55.02 -05:03:21.9 -- not an asteroid (will add it to exclusion list)
19:06:12.84 -03:24:38.2 -- not an asteroid (will add it to exclusion list)
19:12:03.25 +00:53:40.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:32:44.69 -06:06:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:33:07.24 -05:30:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:43:36.09 -06:14:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:45:34.41 -06:17:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:21.80 +00:32:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:48.44 -01:01:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:57.46 +01:36:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:29.67 -00:34:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:53.88 -03:14:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:40.79 -02:21:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:58.44 -02:00:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:20.98 +01:30:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:04:05.26 -03:20:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:59.22 -06:04:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:05.60 -01:30:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:12.84 -03:24:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:38.04 +00:06:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:55.02 -05:03:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:39.98 -05:19:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:51.38 -05:52:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:15.71 -04:11:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:52.95 -04:05:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:09.23 +01:17:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:41.86 -00:04:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:45.42 -03:18:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:00.27 +00:31:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:22.06 -02:50:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:11:59.63 -02:02:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:03.25 +00:53:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:09.24 -03:13:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:10.30 -01:54:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:31.22 -01:10:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:23.01 +02:20:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:42.64 +01:07:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:45.82 -00:16:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:07.77 +02:06:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:08.58 +02:06:11.5 -- 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)
18:32:44.69 -06:06:38.8 -- not a known variable star
18:33:07.24 -05:30:10.5 -- a known variable star
18:43:36.09 -06:14:02.5 -- a known variable star
18:45:34.41 -06:17:18.8 -- a known variable star
18:52:21.80 +00:32:25.0 -- a known variable star
18:52:48.44 -01:01:23.3 -- a known variable star
18:53:57.46 +01:36:35.6 -- a known variable star
18:59:29.67 -00:34:25.3 -- a known variable star
18:59:53.88 -03:14:30.4 -- a known variable star
19:01:40.79 -02:21:00.7 -- a known variable star
19:01:58.44 -02:00:47.5 -- a known variable star
19:02:20.98 +01:30:36.8 -- a known variable star
19:04:05.26 -03:20:39.2 -- a known variable star
19:05:59.22 -06:04:49.3 -- not a known variable star
19:06:05.60 -01:30:00.0 -- a known variable star
19:06:12.84 -03:24:38.2 -- a known variable star
19:06:38.04 +00:06:02.9 -- not a known variable star
19:06:55.02 -05:03:21.9 -- a known variable star
19:07:39.98 -05:19:37.5 -- a known variable star
19:07:51.38 -05:52:36.6 -- a known variable star
19:08:15.71 -04:11:58.8 -- not a known variable star
19:08:52.95 -04:05:48.7 -- a known variable star
19:09:09.23 +01:17:24.1 -- a known variable star
19:09:41.86 -00:04:17.3 -- a known variable star
19:10:45.42 -03:18:46.9 -- a known variable star
19:11:00.27 +00:31:22.0 -- not a known variable star
19:11:22.06 -02:50:25.5 -- not a known variable star
19:11:59.63 -02:02:08.1 -- a known variable star
19:12:03.25 +00:53:40.6 -- a known variable star
19:13:09.24 -03:13:52.1 -- a known variable star
19:13:10.30 -01:54:44.3 -- a known variable star
19:13:31.22 -01:10:47.7 -- not a known variable star
19:14:23.01 +02:20:52.7 -- a known variable star
19:14:42.64 +01:07:53.1 -- a known variable star
19:14:45.82 -00:16:58.5 -- a known variable star
19:15:07.77 +02:06:07.8 -- not a known variable star
19:15:08.58 +02:06:11.5 -- not a known variable star
Found 9 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
37 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 ####
18:32:44.69 -06:06:38.8
18:33:07.24 -05:30:10.5
18:43:36.09 -06:14:02.5
18:45:34.41 -06:17:18.8
18:52:21.80 +00:32:25.0
18:52:48.44 -01:01:23.3
18:53:57.46 +01:36:35.6
18:59:29.67 -00:34:25.3
18:59:53.88 -03:14:30.4
19:01:40.79 -02:21:00.7
19:01:58.44 -02:00:47.5
19:02:20.98 +01:30:36.8
19:04:05.26 -03:20:39.2
19:05:59.22 -06:04:49.3
19:06:05.60 -01:30:00.0
19:06:12.84 -03:24:38.2
19:06:38.04 +00:06:02.9
19:06:55.02 -05:03:21.9
19:07:39.98 -05:19:37.5
19:07:51.38 -05:52:36.6
19:08:15.71 -04:11:58.8
19:08:52.95 -04:05:48.7
19:09:09.23 +01:17:24.1
19:09:41.86 -00:04:17.3
19:10:45.42 -03:18:46.9
19:11:00.27 +00:31:22.0
19:11:22.06 -02:50:25.5
19:11:59.63 -02:02:08.1
19:12:03.25 +00:53:40.6
19:13:09.24 -03:13:52.1
19:13:10.30 -01:54:44.3
19:13:31.22 -01:10:47.7
19:14:23.01 +02:20:52.7
19:14:42.64 +01:07:53.1
19:14:45.82 -00:16:58.5
19:15:07.77 +02:06:07.8
19:15:08.58 +02:06:11.5
18:54:34.92 -00:35:03.8
19:05:41.79 -06:10:44.2
18:56:54.43 -03:07:03.3
19:10:24.71 -03:09:42.9
19:09:23.03 +00:47:09.9
19:12:41.65 +02:10:45.9
19:11:05.06 +01:19:25.5
18:39:44.42 -03:49:15.1
19:09:17.34 -01:41:11.7
19:15:24.96 -03:28:06.2
19:14:02.68 -03:17:27.9
19:01:37.99 -03:33:17.2
19:10:10.49 +01:04:43.4
19:13:56.26 +02:13:01.8
19:03:31.90 -05:44:32.7
19:06:36.75 -05:39:47.4
19:04:04.79 -05:09:17.6
18:43:44.84 -03:16:11.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461132.87010387 -observatory V36
23:05:23.27 -07:28:52.6 Mercury (0.4mag)
02:03:32.17 +12:07:54.5 Venus (-3.9mag)
23:38:57.55 -03:24:30.4 Mars (1.2mag)
07:07:28.47 +22:54:16.4 Jupiter (-2.2mag)
00:23:01.06 +00:10:09.7 Saturn (0.9mag)
03:45:00.43 +19:38:45.0 Uranus (5.8mag)
00:09:00.38 -00:27:00.6 Neptune (7.8mag)
20:32:59.19 -22:52:38.1 Pluto (14.5mag)
12:50:44.39 -09:35:45.7 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 04:06 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461132.87010387:
07:07:36.52 +22:54:00.4 Io (5.7mag)
07:07:40.84 +22:53:52.4 Europa (5.8mag)
07:07:38.20 +22:53:50.4 Ganymede (5.3mag)
07:07:45.00 +22:53:35.3 Callisto (6.5mag)
07:11:18.23 +22:48:50.0 Himalia (15.3mag)
07:07:32.61 +22:54:08.6 Thebe (16.1mag)
07:11:10.25 +23:16:38.3 Elara (17.2mag)
07:05:25.78 +23:41:25.1 Pasiphae (17.3mag)
07:16:04.47 +22:50:42.3 Carme (18.4mag)
00:22:53.72 +00:10:34.7 Titan (8.8mag)
00:22:58.79 +00:10:17.3 Rhea (10.1mag)
00:23:10.35 +00:12:05.2 Iapetus (11.5mag)
00:22:51.44 +00:10:18.0 Hyperion (14.8mag)
00:24:47.88 +00:20:20.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 04:06 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.87010387:
14:22:21.09 -04:37:00.1 JWST
19:44:56.86 +06:44:19.9 Chandra
08:32:38.69 -47:08:37.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 04:06 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.87010387 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:45.01 -28:02:27.0 14.0mag P/2010 H2 (Vales)
04:57:44.08 -70:20:55.0 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.21 +31:21:18.1 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.74 +08:54:19.9 17.6mag C/2021 G2 (ATLAS)
23:06:05.55 +28:44:45.1 17.0mag C/2022 E2 (ATLAS)
04:13:43.93 +25:39:14.0 15.9mag C/2022 N2 (PANSTARRS)
09:01:34.80 +31:49:50.9 16.1mag C/2022 QE78 (ATLAS)
08:29:48.55 -01:40:32.1 17.2mag C/2022 R6 (PANSTARRS)
18:56:02.53 +17:21:47.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:24.06 -11:42:37.6 17.6mag P/2023 B1 (PANSTARRS)
09:15:14.93 -14:09:30.6 17.5mag C/2023 F3 (ATLAS)
21:38:47.15 +62:11:15.4 17.4mag C/2023 H5 (Lemmon)
19:28:32.45 -03:34:41.2 14.3mag C/2023 R1 (PANSTARRS)
21:42:54.85 +84:08:52.0 17.8mag C/2023 X2 (Lemmon)
06:13:57.67 +63:37:28.3 17.0mag C/2024 A1 (ATLAS)
04:41:36.50 +12:45:49.1 10.1mag C/2024 E1 (Wierzchos)
16:27:04.71 +04:09:04.5 17.4mag C/2024 G6 (ATLAS)
20:15:59.94 +11:43:04.9 14.8mag C/2024 J3 (ATLAS)
03:14:32.79 -24:32:48.7 16.4mag C/2024 T5 (ATLAS)
05:05:48.05 +48:53:34.3 17.6mag C/2025 J1 (Borisov)
14:33:48.14 +33:16:48.8 14.7mag C/2025 L1 (ATLAS)
03:04:54.42 -24:12:50.2 17.7mag C/2025 Q3 (ATLAS)
22:45:36.84 +19:45:16.5 10.7mag C/2025 R3 (PANSTARRS)
13:00:02.28 +02:08:23.2 17.5mag C/2025 Y1 (ATLAS)
01:20:45.27 +02:40:23.8 8.4mag C/2026 A1 (MAPS)
23:19:02.85 +34:21:59.5 14.1mag C/2026 B2 (Sun-Gao)
18:16:18.60 -10:23:31.5 12.6mag 10P/Tempel
15:17:09.20 +04:23:56.1 12.8mag 24P/Schaumasse
11:07:06.74 -02:00:20.2 15.7mag 29P/Schwassmann-Wachmann
17:54:20.56 -10:08:59.9 17.6mag 40P/Vaisala
10:39:55.37 -05:18:49.9 16.6mag 43P/Wolf-Harrington
01:27:42.34 +15:07:33.8 17.1mag 47P/Ashbrook-Jackson
06:46:59.09 +39:51:54.6 17.1mag 63P/Wild
23:11:12.44 -13:08:17.0 15.7mag 65P/Gunn
03:28:05.58 +16:17:11.3 15.8mag 76P/West-Kohoutek-Ikemura
00:35:49.40 +05:31:17.5 14.5mag 78P/Gehrels
22:20:14.66 -13:22:12.1 14.5mag 88P/Howell
01:32:53.02 +16:51:25.0 15.1mag 93P/Lovas
04:30:20.53 +31:29:30.1 16.3mag 123P/West-Hartley
08:14:37.31 +44:39:04.8 16.2mag 124P/Mrkos
02:12:28.78 +12:48:48.7 16.4mag 128P/Shoemaker-Holt
02:21:00.81 +12:44:49.3 17.4mag 131P/Mueller
00:17:08.46 +08:05:41.8 11.6mag 141P/Machholz
00:27:18.98 -00:11:58.1 11.6mag 141P-A/Machholz
23:20:11.57 -03:35:18.8 14.5mag 141P-D/Machholz
00:55:45.73 +01:23:31.2 18.0mag 141P-I/Machholz
00:24:34.70 -08:17:19.9 15.3mag 162P/SidingSpring
10:32:24.29 +31:42:30.9 17.7mag 164P/Christensen
06:11:29.63 +24:36:04.1 17.8mag 198P/ODAS
15:15:07.45 -01:41:21.1 17.2mag 210P/Christensen
20:56:19.61 -14:44:14.7 17.3mag 218P/LINEAR
17:10:11.52 -15:29:16.8 16.2mag 235P/LINEAR
05:05:47.46 +33:28:07.5 16.5mag 240P/NEAT
07:32:51.38 -06:45:19.3 17.6mag 242P/Spahr
15:46:53.29 +06:01:43.1 17.6mag 391P/Kowalski
07:29:56.39 +21:16:34.0 17.6mag 450P/LONEOS
05:16:42.93 +45:50:27.3 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 04:06 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
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
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
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
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
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
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
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
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
-rw-r--r-- 1 apache apache 5.8K Apr 2 04:06 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
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
-rw-r--r-- 1 apache apache 187K Apr 2 04:06 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:08:11.420 -04:49:30.53 AT 2026hkf 2026-03-14.22 21.0121
04:20:57.978 -04:44:24.49 AT 2026hke 2026-03-26.13 19.8012
08:08:20.226 -14:40:00.64 AT 2026hkd 2026-03-07.19 20.1897
07:59:24.647 +57:00:58.39 AT 2026hkc 2026-03-14.20 20.9477
13:58:50.252 -17:03:03.26 AT 2026hkb 2026-03-23.24 19.315
08:55:52.185 -18:24:10.01 AT 2026hka 2026-03-20.39 19.87
19:49:11.846 -17:41:20.03 AT 2026hjz 2026-03-24.76 19.09
17:23:18.071 +42:30:08.80 AT 2026hjy 2026-03-15.19 19.329
15:36:56.914 -04:11:42.38 AT 2026hjx 2026-03-25.78 20.01
16:12:19.428 -02:04:41.40 AT 2026hjw 2026-03-24.64 20.22
11:18:56.464 -28:36:26.32 AT 2026hjv 2026-03-21.92 19.08
13:33:46.392 +11:46:20.90 AT 2026hju 2026-03-20.24 18.89
11:08:39.309 -42:07:08.38 AT 2026hjt 2026-03-25.18 19.306
18:40:00.884 -46:00:21.86 AT 2026hjs 2026-03-22.37 19.141
10:49:28.071 -32:24:01.15 AT 2026hjr 2026-03-21.92 19.476
08:13:57.386 +50:00:46.26 AT 2026hjq 2026-03-08.96 20.035
18:55:05.624 -41:25:59.25 AT 2026hjp 2026-03-24.79 20.17
14:10:06.186 +10:00:51.42 AT 2026hjo 2026-03-24.40 20.2791
08:47:29.260 +16:55:56.97 AT 2026hjn 2026-03-20.25 20.8588
08:53:19.672 -26:00:27.80 AT 2026hjm 2026-03-26.19 19.4129
-rw-r--r-- 1 apache apache 29K Apr 2 04:06 tns_transients_list.txt
