This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4206254677782798080,2461144.8314,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4206254677782798080 20260414.3314 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1850044-053839,2461144.8314,12.74,0.05,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_J1850044-053839 20260414.3314 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190037.68-035025.6,2461144.8314,12.61,0.05,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
ASASSN-V J190037.68-035025.6 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1859293+020043,2461144.8314,12.76,0.05,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
NSVS J1859293+020043 20260414.3314 12.76CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185939.84-044702.3,2461144.8314,12.55,0.05,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
ASASSN-V J185939.84-044702.3 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1901237-020506,2461144.8314,12.48,0.05,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_J1901237-020506 20260414.3314 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13963982,2461144.8314,12.76,0.05,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
NSVS 13963982 20260414.3314 12.76CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1843261-051144,2461144.8314,12.23,0.05,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_J1843261-051144 20260414.3314 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1902334-024121,2461144.8314,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1902334-024121 20260414.3314 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13963876,2461144.8314,12.59,0.05,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 13963876 20260414.3314 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190519.28-014219.4,2461144.8314,12.61,0.05,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
ASASSN-V J190519.28-014219.4 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FASTT 1196,2461144.8314,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FASTT 1196 20260414.3314 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13960229,2461144.8314,11.31,0.05,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 13960229 20260414.3314 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13949520,2461144.8314,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13949520 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1849486-043240,2461144.8314,12.69,0.05,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
GDS_J1849486-043240 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1852562-040644,2461144.8314,12.95,0.05,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_J1852562-040644 20260414.3314 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1854306-042353,2461144.8314,12.79,0.05,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_J1854306-042353 20260414.3314 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1853478-043403,2461144.8314,12.53,0.05,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
GDS_J1853478-043403 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185547.16-054749.3,2461144.8314,12.04,0.05,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
ASASSN-V J185547.16-054749.3 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13985056,2461144.8314,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13985056 20260414.3314 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190611.83-043154.0,2461144.8314,12.37,0.05,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 J190611.83-043154.0 20260414.3314 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185641.09-042526.9,2461144.8314,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185641.09-042526.9 20260414.3314 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 14.3315* 18 27 38.10 -02 35 57.2 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1827379-023558,2461144.8314,12.44,0.05,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 J1827379-023558 20260414.3314 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185914.15-043752.1,2461144.8314,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185914.15-043752.1 20260414.3314 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185328.68+012156.8,2461144.8314,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185328.68+012156.8 20260414.3314 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1851374-032610,2461144.8314,12.87,0.05,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_J1851374-032610 20260414.3314 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13983865,2461144.8314,12.37,0.05,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 13983865 20260414.3314 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 11402,2461144.8314,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 11402 20260414.3314 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1900567-005932,2461144.8314,12.60,0.05,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_J1900567-005932 20260414.3314 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1858104-032641,2461144.8314,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1858104-032641 20260414.3314 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 14.3315* 18 36 58.84 -02 08 49.3 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13938607,2461144.8314,12.37,0.05,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 13938607 20260414.3314 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1902143-001908,2461144.8314,12.74,0.05,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_J1902143-001908 20260414.3314 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J19061358+0216209,2461144.8314,12.06,0.05,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
2MASS J19061358+0216209 20260414.3314 12.06CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1855159-024608,2461144.8314,12.55,0.05,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_J1855159-024608 20260414.3314 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190334.01-052323.3,2461144.8314,12.19,0.05,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
ASASSN-V J190334.01-052323.3 20260414.3314 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
## 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: 2461144.83177094 14.04.2026 07:57:35.009 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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): 8458
Objects passed selection criteria: 8427
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 6293.25
Average stars matched: 6101.75 (96.9571 %)
Memory usage VmPeak: 115544 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 03:02:33 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: 2461144.83177094 14.04.2026 07:57:35.009 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 169
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: 27 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): 102480
Objects passed selection criteria: 102179
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 73819.2
Average stars matched: 70401.5 (95.3701 %)
Memory usage VmPeak: 2294216 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 03:05:05 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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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: 2461144.83112152
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits'
wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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 18:51:20.420 -01:59:04.17
Angular distance between the image centers 0.0245 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 18:51:22.996 -01:58:54.23
Angular distance between the image centers 0.0193 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 18:51:20.420 -01:59:04.17
Second-epoch second image center 18:51:22.996 -01:58:54.23
Angular distance between the image centers 0.01108 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.ZMa7MY9vMz
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.EVC4jrtuVS
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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits &> /tmp/tmp.RQkXEi9MZd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits &> /tmp/tmp.H5A9c5g0Gu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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
2.9 pix fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
2.9 pix fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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
13.1 mag. fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
13.2 mag. fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.8 (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.ZMa7MY9vMz (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EVC4jrtuVS (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RQkXEi9MZd (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=246, passed=3993
Got 3993 stars (including 3745 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat
util/solve_plate_with_UCAC5 got 3993 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 3912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 3910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 3910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 933 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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.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.H5A9c5g0Gu (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=263, passed=4315
Got 4315 stars (including 4048 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat
util/solve_plate_with_UCAC5 got 4315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 4245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 4246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 4246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11029_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 11029_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:21.01 +01:30:38.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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 18:51:20.420 -01:59:04.17
Angular distance between the image centers 0.0245 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 18:51:22.996 -01:58:54.23
Angular distance between the image centers 0.0193 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 18:51:20.420 -01:59:04.17
Second-epoch second image center 18:51:22.996 -01:58:54.23
Angular distance between the image centers 0.01108 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.sxs5I9bRQf
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.xPz0rOZNqO
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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits &> /tmp/tmp.JPFP6iW9ff
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits &> /tmp/tmp.CKPDocyJBU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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 125 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.1 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
2.6 pix fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
2.5 pix fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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
13.4 mag. fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
13.5 mag. fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 13.0 (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.sxs5I9bRQf (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xPz0rOZNqO (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JPFP6iW9ff (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2392, passed=37402
Got 37402 stars (including 34970 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat
util/solve_plate_with_UCAC5 got 37402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 36615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 36612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 36613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.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.CKPDocyJBU (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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=2662, passed=40228
Got 40228 stars (including 37516 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat
util/solve_plate_with_UCAC5 got 40228 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 39516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 39516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 39516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/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_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-56-38_20.00sec_-4.90C_LIGHT_0856.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.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_2026-04-14_CI_Aql-03-Q2b1x1_025828_TTUQ2b1x1_28306_B4wY6jGm/wcs_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out101137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out36470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out92818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out103362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92194.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 16s
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Considering the candidate 177227_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177227_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:55:40.20 -06:04:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.112 4253975926361890560 283.91780382796 -06.07844732669 12.6826 11.6935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177239_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177239_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:58:47.46 -04:23:21.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)
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Considering the candidate 177240_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177240_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:05:04.22 -00:14:03.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
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Considering the candidate 177252_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 177252_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 177255_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177255_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:06:16.78 -05:15:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 2.294 4206321374361186688 286.56951239250 -05.25349392620 11.5978 11.0114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177285_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177285_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:58.59 -03:43:12.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177291_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177291_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:57:03.65 -05:49:05.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177300_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177300_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:04:20.91 -05:42:47.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177303_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177303_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:33.71 -05:43:08.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 177306_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177306_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:47:27.28 -05:43:49.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177315_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177315_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:07:43.93 -02:25:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177317_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177317_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:33:07.17 -05:08:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.045 4256447937661957248 278.27955342509 -05.14283636689 12.7449 12.0711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177325_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177325_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:05:13.37 +01:52:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177336_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177336_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:07:37.26 +00:06:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177341_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177341_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:05:31.55 -00:39:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177343_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177343_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:59:30.45 -05:14:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177345_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177345_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:24:32.37 -01:32:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177346_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177346_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:08:04.19 -03:50:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177352_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 177352_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:05:21.21 -03:18:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32297_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 32297_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:47:28.99 -05:42:16.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 59831_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 59831_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:04:57.32 -04:01:58.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84941_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 84941_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:09:06.56 -02:14:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36284_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 36284_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 65617_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 65617_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 115835_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 115835_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:53:57.46 +01:36:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150785_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 150785_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 92818_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 92818_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:00:25.33 -01:40:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 5.647 4262052075393360512 285.10526959419 -01.67929484288 12.3595 11.0426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 39045_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 39045_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:33:07.32 -05:30:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52097_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 52097_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 87228_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 87228_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 60170_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 60170_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 84001_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 84001_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:58:41.73 -02:20:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45015_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 45015_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 79475_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 79475_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 87924_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 87924_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:58.43 -02:00:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84634_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 84634_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:58:42.99 -02:16:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103890_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 103890_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:51:53.72 -00:58:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49202_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 49202_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 44410_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 44410_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:45:44.68 -05:14:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73075_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 73075_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:52:35.89 -03:12:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74720_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 74720_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:04:01.04 -03:05:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22456_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 22456_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:47:21.42 -06:16:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85292_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 85292_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:40.32 -02:11:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99382_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 99382_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:06:05.38 -01:12:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70335_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 70335_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:43:24.51 -03:30:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92194_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 92194_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 125106_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 125106_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 25563_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 25563_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 39715_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 39715_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 139263_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 139263_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:59:29.65 -00:34:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61778_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 61778_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:08:52.90 -04:05:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55665_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 55665_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 71757_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 71757_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:04:05.24 -03:20:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62374_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 62374_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 58254_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 58254_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 142804_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 142804_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:05:52.11 -00:49:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55496_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 55496_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 70668_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 70668_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:06:12.80 -03:24:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45130_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 45130_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:04:04.77 -05:09:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126971_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 126971_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:56.70 +00:25:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83700_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 83700_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:40.76 -02:21:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95332_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 95332_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:06:05.46 -01:29:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49595_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 49595_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:37:12.99 -04:57:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165533_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 165533_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:56:26.46 -00:58:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73022_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 73022_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:59:53.74 -03:14:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165407_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 165407_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:05:41.77 -06:10:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73000_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 73000_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:43:44.71 -03:16:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32863_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 32863_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 147796_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 147796_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:40.02 +02:11:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142326_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 142326_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:58:34.38 -00:47:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57707_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 57707_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:39.34 -04:19:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73869_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 73869_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:05.02 -03:10:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103039_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 103039_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:52:48.41 -01:01:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56873_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 56873_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 165073_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 165073_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:09:00.97 +00:21:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35089_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 35089_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:43:01.49 -05:42:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32562_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 32562_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:56:55.39 -05:48:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131573_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 131573_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:04:28.02 +00:03:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92087_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 92087_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:58:01.61 -01:43:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55734_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 55734_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
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Considering the candidate 33038_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 33038_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:55:16.89 -05:47:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146304_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 146304_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:53:14.17 +02:15:40.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75227_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 75227_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:08:59.23 -03:01:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146876_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 146876_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:20.97 +01:30:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57791_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 57791_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143450_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 143450_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:48.14 -00:52:31.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26928_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 26928_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:49:55.03 -06:04:31.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101137_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 101137_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:33.64 -01:07:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.530 4262471401641458944 285.64001928269 -01.12194521318 11.2906 9.7583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81025_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 81025_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83983_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 83983_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:42:23.79 -02:22:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54577_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 54577_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152718_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 152718_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173105_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 173105_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:03:24.70 -00:32:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71054_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 71054_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75011_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 75011_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41887_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 41887_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:07:39.96 -05:19:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95394_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 95394_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:42.80 -01:30:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98233_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 98233_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:59:11.44 -01:19:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23629_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 23629_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36470_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 36470_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:47:40.56 -05:38:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.206 4253359924975405824 281.91849390320 -05.63832126362 10.9225 9.4986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83576_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 83576_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:08:00.25 -02:19:19.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103362_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 103362_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167514_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 167514_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28067_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 28067_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:07:38.65 -05:58:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56749_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 56749_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:49:15.67 -04:29:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86788_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 86788_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136619_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 136619_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83973_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 83973_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:07:13.09 -02:18:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22207_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 22207_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:45:34.15 -06:17:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146361_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 146361_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78666_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 78666_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31962_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 31962_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:08:37.26 -05:48:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31955_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 31955_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:09:12.31 -05:48:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41503_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 41503_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:56:04.71 -05:21:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71356_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 71356_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:51:22.18 -03:19:04.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40791_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
Preparing report for the candidate 40791_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46681_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 46681_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:06:55.02 -05:03:21.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48755_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 48755_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:47:10.60 -04:44:50.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65883_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 65883_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:02:54.41 -03:41:55.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30271_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 30271_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:49:40.99 -05:54:45.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28954_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 28954_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 18:57:03.69 -05:50:44.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31401_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 31401_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:01:40.60 -05:44:18.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32052_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 32052_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:04:24.07 -05:41:05.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46207_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 46207_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:06:14.66 -04:52:57.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120708_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857
The candidate 120708_fd_Aql-03-Q2b1x1_2026-04-14_02-57-35_20.00sec_-5.00C_LIGHT_0857 did not pass the final checks
**** FOUND 19:03:32.21 +01:49:03.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 36s
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 ####
19:00:56.43 -00:59:33.2
19:02:41.43 +00:36:13.5
19:02:14.24 -00:19:07.5
19:06:13.36 +02:16:14.2
18:59:29.04 +02:00:36.8
18:53:28.71 +01:21:54.7
18:58:10.04 -03:26:39.1
19:07:24.03 -05:29:06.8
18:50:38.94 -06:13:09.4
18:53:58.35 -06:09:18.3
18:55:47.20 -05:47:48.3
18:50:04.55 -05:38:37.3
18:45:51.48 -05:28:46.7
19:03:33.91 -05:23:21.2
18:43:25.88 -05:11:44.5
18:56:29.10 -04:57:26.2
18:59:39.83 -04:47:00.1
18:59:14.12 -04:37:49.6
18:53:47.75 -04:34:02.5
18:49:48.74 -04:32:39.5
19:06:11.75 -04:31:51.8
19:09:24.49 -04:26:52.2
18:56:41.24 -04:25:24.7
18:54:30.41 -04:23:54.7
18:56:33.10 -04:15:17.5
18:52:56.27 -04:06:45.1
19:00:37.67 -03:50:22.9
18:51:37.42 -03:26:09.9
19:08:39.11 -03:02:07.8
18:55:14.90 -02:46:08.7
19:02:33.28 -02:41:22.7
18:27:38.10 -02:35:57.2
18:36:58.84 -02:08:49.3
19:01:23.72 -02:05:09.1
19:05:19.14 -01:42:19.7
########### 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 ####
19:07:24.03 -05:29:06.8
18:50:04.55 -05:38:37.3
19:00:37.67 -03:50:22.9
18:59:29.04 +02:00:36.8
18:59:39.83 -04:47:00.1
19:01:23.72 -02:05:09.1
18:56:33.10 -04:15:17.5
18:43:25.88 -05:11:44.5
19:02:33.28 -02:41:22.7
18:56:29.10 -04:57:26.2
19:05:19.14 -01:42:19.7
19:02:41.43 +00:36:13.5
18:53:58.35 -06:09:18.3
18:45:51.48 -05:28:46.7
18:49:48.74 -04:32:39.5
18:52:56.27 -04:06:45.1
18:54:30.41 -04:23:54.7
18:53:47.75 -04:34:02.5
18:55:47.20 -05:47:48.3
19:09:24.49 -04:26:52.2
19:06:11.75 -04:31:51.8
18:56:41.24 -04:25:24.7
18:27:38.10 -02:35:57.2
18:59:14.12 -04:37:49.6
18:53:28.71 +01:21:54.7
18:51:37.42 -03:26:09.9
19:08:39.11 -03:02:07.8
18:50:38.94 -06:13:09.4
19:00:56.43 -00:59:33.2
18:58:10.04 -03:26:39.1
18:36:58.84 -02:08:49.3
19:02:14.24 -00:19:07.5
19:06:13.36 +02:16:14.2
18:55:14.90 -02:46:08.7
19:03:33.91 -05:23:21.2
###################################################################################
19:07:24.03 -05:29:06.8 -- not an asteroid (will add it to exclusion list)
18:50:04.55 -05:38:37.3 -- not an asteroid (will add it to exclusion list)
19:00:37.67 -03:50:22.9 -- not an asteroid (will add it to exclusion list)
18:59:29.04 +02:00:36.8 -- not an asteroid (will add it to exclusion list)
18:59:39.83 -04:47:00.1 -- not an asteroid (will add it to exclusion list)
19:01:23.72 -02:05:09.1 -- not an asteroid (will add it to exclusion list)
18:56:33.10 -04:15:17.5 -- not an asteroid (will add it to exclusion list)
18:43:25.88 -05:11:44.5 -- not an asteroid (will add it to exclusion list)
19:02:33.28 -02:41:22.7 -- not an asteroid (will add it to exclusion list)
18:56:29.10 -04:57:26.2 -- not an asteroid (will add it to exclusion list)
19:05:19.14 -01:42:19.7 -- not an asteroid (will add it to exclusion list)
19:02:41.43 +00:36:13.5 -- not an asteroid (will add it to exclusion list)
18:53:58.35 -06:09:18.3 -- not an asteroid (will add it to exclusion list)
18:45:51.48 -05:28:46.7 -- not an asteroid (will add it to exclusion list)
18:49:48.74 -04:32:39.5 -- not an asteroid (will add it to exclusion list)
18:52:56.27 -04:06:45.1 -- not an asteroid (will add it to exclusion list)
18:54:30.41 -04:23:54.7 -- not an asteroid (will add it to exclusion list)
18:53:47.75 -04:34:02.5 -- not an asteroid (will add it to exclusion list)
18:55:47.20 -05:47:48.3 -- not an asteroid (will add it to exclusion list)
19:09:24.49 -04:26:52.2 -- not an asteroid (will add it to exclusion list)
19:06:11.75 -04:31:51.8 -- not an asteroid (will add it to exclusion list)
18:56:41.24 -04:25:24.7 -- not an asteroid (will add it to exclusion list)
18:27:38.10 -02:35:57.2 -- not an asteroid (will add it to exclusion list)
18:59:14.12 -04:37:49.6 -- not an asteroid (will add it to exclusion list)
18:53:28.71 +01:21:54.7 -- not an asteroid (will add it to exclusion list)
18:51:37.42 -03:26:09.9 -- not an asteroid (will add it to exclusion list)
19:08:39.11 -03:02:07.8 -- not an asteroid (will add it to exclusion list)
18:50:38.94 -06:13:09.4 -- not an asteroid (will add it to exclusion list)
19:00:56.43 -00:59:33.2 -- not an asteroid (will add it to exclusion list)
18:58:10.04 -03:26:39.1 -- not an asteroid (will add it to exclusion list)
18:36:58.84 -02:08:49.3 -- not an asteroid (will add it to exclusion list)
19:02:14.24 -00:19:07.5 -- not an asteroid (will add it to exclusion list)
19:06:13.36 +02:16:14.2 -- not an asteroid (will add it to exclusion list)
18:55:14.90 -02:46:08.7 -- not an asteroid (will add it to exclusion list)
19:03:33.91 -05:23:21.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:27:38.10 -02:35:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:36:58.84 -02:08:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:43:25.88 -05:11:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:45:51.48 -05:28:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:48.74 -04:32:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:04.55 -05:38:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:38.94 -06:13:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:37.42 -03:26:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:56.27 -04:06:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:28.71 +01:21:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:47.75 -04:34:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:58.35 -06:09:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:30.41 -04:23:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:14.90 -02:46:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:47.20 -05:47:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:29.10 -04:57:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:33.10 -04:15:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:41.24 -04:25:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:10.04 -03:26:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:14.12 -04:37:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:29.04 +02:00:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:39.83 -04:47:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:37.67 -03:50:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:56.43 -00:59:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:23.72 -02:05:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:14.24 -00:19:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:33.28 -02:41:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:41.43 +00:36:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:33.91 -05:23:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:19.14 -01:42:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:11.75 -04:31:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:13.36 +02:16:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:24.03 -05:29:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:39.11 -03:02:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:24.49 -04:26:52.2 -- 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)
18:27:38.10 -02:35:57.2 -- a known variable star
18:36:58.84 -02:08:49.3 -- a known variable star
18:43:25.88 -05:11:44.5 -- a known variable star
18:45:51.48 -05:28:46.7 -- a known variable star
18:49:48.74 -04:32:39.5 -- a known variable star
18:50:04.55 -05:38:37.3 -- a known variable star
18:50:38.94 -06:13:09.4 -- a known variable star
18:51:37.42 -03:26:09.9 -- a known variable star
18:52:56.27 -04:06:45.1 -- a known variable star
18:53:28.71 +01:21:54.7 -- a known variable star
18:53:47.75 -04:34:02.5 -- a known variable star
18:53:58.35 -06:09:18.3 -- a known variable star
18:54:30.41 -04:23:54.7 -- a known variable star
18:55:14.90 -02:46:08.7 -- a known variable star
18:55:47.20 -05:47:48.3 -- a known variable star
18:56:29.10 -04:57:26.2 -- a known variable star
18:56:33.10 -04:15:17.5 -- a known variable star
18:56:41.24 -04:25:24.7 -- a known variable star
18:58:10.04 -03:26:39.1 -- a known variable star
18:59:14.12 -04:37:49.6 -- a known variable star
18:59:29.04 +02:00:36.8 -- a known variable star
18:59:39.83 -04:47:00.1 -- a known variable star
19:00:37.67 -03:50:22.9 -- a known variable star
19:00:56.43 -00:59:33.2 -- a known variable star
19:01:23.72 -02:05:09.1 -- a known variable star
19:02:14.24 -00:19:07.5 -- a known variable star
19:02:33.28 -02:41:22.7 -- a known variable star
19:02:41.43 +00:36:13.5 -- a known variable star
19:03:33.91 -05:23:21.2 -- a known variable star
19:05:19.14 -01:42:19.7 -- a known variable star
19:06:11.75 -04:31:51.8 -- a known variable star
19:06:13.36 +02:16:14.2 -- a known variable star
19:07:24.03 -05:29:06.8 -- not a known variable star
19:08:39.11 -03:02:07.8 -- a known variable star
19:09:24.49 -04:26:52.2 -- a known variable star
Found 1 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
35 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 ####
18:27:38.10 -02:35:57.2
18:36:58.84 -02:08:49.3
18:43:25.88 -05:11:44.5
18:45:51.48 -05:28:46.7
18:49:48.74 -04:32:39.5
18:50:04.55 -05:38:37.3
18:50:38.94 -06:13:09.4
18:51:37.42 -03:26:09.9
18:52:56.27 -04:06:45.1
18:53:28.71 +01:21:54.7
18:53:47.75 -04:34:02.5
18:53:58.35 -06:09:18.3
18:54:30.41 -04:23:54.7
18:55:14.90 -02:46:08.7
18:55:47.20 -05:47:48.3
18:56:29.10 -04:57:26.2
18:56:33.10 -04:15:17.5
18:56:41.24 -04:25:24.7
18:58:10.04 -03:26:39.1
18:59:14.12 -04:37:49.6
18:59:29.04 +02:00:36.8
18:59:39.83 -04:47:00.1
19:00:37.67 -03:50:22.9
19:00:56.43 -00:59:33.2
19:01:23.72 -02:05:09.1
19:02:14.24 -00:19:07.5
19:02:33.28 -02:41:22.7
19:02:41.43 +00:36:13.5
19:03:33.91 -05:23:21.2
19:05:19.14 -01:42:19.7
19:06:11.75 -04:31:51.8
19:06:13.36 +02:16:14.2
19:07:24.03 -05:29:06.8
19:08:39.11 -03:02:07.8
19:09:24.49 -04:26:52.2
19:02:33.64 -01:07:19.0
19:01:48.14 -00:52:31.9
18:55:40.20 -06:04:40.6
18:58:47.46 -04:23:21.5
19:05:04.22 -00:14:03.6
19:06:16.78 -05:15:10.8
18:33:07.17 -05:08:35.9
18:47:40.56 -05:38:16.7
19:00:25.33 -01:40:39.9
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461144.83112152 -observatory V36
23:58:36.10 -02:57:08.1 Mercury (0.1mag)
03:00:30.51 +17:13:19.0 Venus (-3.9mag)
00:13:06.19 +00:20:34.5 Mars (1.2mag)
07:11:53.15 +22:47:26.3 Jupiter (-2.1mag)
00:28:26.22 +00:44:19.9 Saturn (0.9mag)
03:47:20.87 +19:46:21.2 Uranus (5.8mag)
00:10:37.29 -00:16:45.1 Neptune (7.8mag)
20:33:40.77 -22:52:31.8 Pluto (14.5mag)
22:56:55.10 -06:59:39.9 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 361 Apr 14 03:02 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461144.83112152:
07:11:54.02 +22:47:27.0 Io (5.8mag)
07:11:48.43 +22:47:33.4 Europa (5.9mag)
07:12:04.13 +22:47:09.7 Ganymede (5.3mag)
07:12:20.86 +22:46:36.2 Callisto (6.6mag)
07:15:17.74 +22:35:50.8 Himalia (15.3mag)
07:11:51.89 +22:47:31.1 Thebe (16.2mag)
07:15:26.95 +23:05:54.4 Elara (17.3mag)
07:10:39.24 +23:28:19.0 Pasiphae (17.4mag)
07:20:15.08 +22:45:17.6 Carme (18.5mag)
00:28:33.69 +00:44:37.2 Titan (8.8mag)
00:28:27.31 +00:44:34.9 Rhea (10.1mag)
00:28:09.23 +00:44:45.3 Iapetus (11.5mag)
00:28:39.19 +00:44:29.8 Hyperion (14.8mag)
00:30:04.44 +00:53:18.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 14 03:02 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.83112152:
15:30:16.32 -15:05:48.4 JWST
17:19:13.60 +43:00:24.9 Chandra
08:29:55.17 -46:41:03.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 14 03:02 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.83112152 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:18.28 -28:40:55.1 13.9mag P/2010 H2 (Vales)
05:05:32.67 -69:44:28.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:05.40 +31:25:33.8 17.2mag C/2017 K2 (PANSTARRS)
17:30:35.46 +10:20:59.1 17.6mag C/2021 G2 (ATLAS)
23:09:46.60 +29:09:47.5 17.1mag C/2022 E2 (ATLAS)
04:27:17.71 +25:59:34.4 16.0mag C/2022 N2 (PANSTARRS)
09:03:04.25 +32:00:24.4 16.2mag C/2022 QE78 (ATLAS)
08:30:49.40 -00:19:49.7 17.3mag C/2022 R6 (PANSTARRS)
18:54:07.18 +18:23:31.9 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:12.52 -11:32:45.8 17.5mag P/2023 B1 (PANSTARRS)
09:08:25.12 -12:09:04.4 17.6mag C/2023 F3 (ATLAS)
21:52:31.62 +62:48:33.9 17.5mag C/2023 H5 (Lemmon)
19:20:37.14 -03:42:20.8 14.2mag C/2023 R1 (PANSTARRS)
21:35:38.99 +85:40:51.7 17.8mag C/2023 X2 (Lemmon)
06:17:08.39 +63:31:13.8 17.1mag C/2024 A1 (ATLAS)
05:09:40.54 +17:44:37.7 10.9mag C/2024 E1 (Wierzchos)
16:20:20.47 +06:07:00.8 17.4mag C/2024 G6 (ATLAS)
20:20:20.21 +14:49:20.5 14.6mag C/2024 J3 (ATLAS)
03:24:52.41 -22:38:24.5 16.4mag C/2024 T5 (ATLAS)
05:15:18.07 +45:42:24.3 17.7mag C/2025 J1 (Borisov)
13:45:45.85 +44:22:05.3 15.1mag C/2025 L1 (ATLAS)
03:22:38.91 -25:57:07.7 17.8mag C/2025 Q3 (ATLAS)
23:29:54.94 +19:06:18.5 8.8mag C/2025 R3 (PANSTARRS)
12:54:50.44 +02:54:39.5 17.4mag C/2025 Y1 (ATLAS)
03:13:38.12 +02:48:50.6 12.8mag C/2026 A1 (MAPS)
23:54:50.06 +36:54:34.1 14.5mag C/2026 B2 (Sun-Gao)
18:39:41.23 -09:48:30.7 11.9mag 10P/Tempel
15:02:33.20 +03:22:52.2 13.8mag 24P/Schaumasse
11:03:15.15 -01:34:48.8 15.7mag 29P/Schwassmann-Wachmann
18:00:27.48 -09:40:19.4 17.9mag 40P/Vaisala
10:37:38.69 -04:13:57.2 16.9mag 43P/Wolf-Harrington
01:46:05.51 +17:12:10.5 17.2mag 47P/Ashbrook-Jackson
07:07:41.46 +37:22:13.7 17.0mag 63P/Wild
23:26:55.64 -11:39:06.0 15.7mag 65P/Gunn
03:58:47.96 +20:40:44.8 15.9mag 76P/West-Kohoutek-Ikemura
01:01:53.33 +07:54:01.9 14.3mag 78P/Gehrels
22:57:56.52 -09:53:05.0 14.6mag 88P/Howell
02:05:41.14 +20:11:46.5 15.1mag 93P/Lovas
04:51:39.94 +32:11:53.0 16.2mag 123P/West-Hartley
08:26:24.56 +39:07:50.2 16.2mag 124P/Mrkos
02:30:38.34 +14:11:00.9 16.4mag 128P/Shoemaker-Holt
02:44:15.90 +14:17:20.5 17.5mag 131P/Mueller
01:17:24.92 +12:39:27.8 10.7mag 141P/Machholz
01:26:34.43 +04:14:50.3 10.7mag 141P-A/Machholz
00:12:40.73 +00:13:08.3 13.0mag 141P-D/Machholz
01:56:45.50 +06:00:03.3 17.8mag 141P-I/Machholz
00:57:43.61 -02:21:54.5 15.1mag 162P/SidingSpring
10:29:04.51 +30:56:41.0 18.0mag 164P/Christensen
06:33:26.80 +24:17:37.7 18.0mag 198P/ODAS
14:54:23.83 -00:14:31.2 17.6mag 210P/Christensen
21:33:59.99 -11:51:04.4 17.6mag 218P/LINEAR
17:16:07.47 -14:08:01.5 16.1mag 235P/LINEAR
05:30:52.87 +34:34:14.5 16.7mag 240P/NEAT
07:37:40.75 -05:20:54.9 17.7mag 242P/Spahr
22:12:44.41 -21:25:19.1 17.9mag 260P/McNaught
15:43:17.24 +06:52:48.2 17.5mag 391P/Kowalski
07:33:33.65 +21:21:37.7 17.7mag 450P/LONEOS
05:33:26.41 +45:07:48.4 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 14 03:02 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
-rw-r--r-- 1 apache apache 5.8K Apr 14 03:02 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
-rw-r--r-- 1 apache apache 188K Apr 14 03:02 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:08:01.002 +67:05:08.73 AT 2026ivq 2026-04-04.49 19.4548
18:36:22.696 +81:45:06.35 AT 2026ivp 2026-03-27.51 20.7475
15:19:48.489 -05:00:11.22 AT 2026ivo 2026-03-27.48 21.2654
15:56:56.656 +27:09:01.74 AT 2026ivn 2026-04-04.38 19.6722
13:56:43.855 -19:49:48.79 AT 2026ivm 2026-04-07.40 19.7776
09:53:53.828 +01:43:05.64 AT 2026ivl 2026-04-07.17 22.04
11:56:09.924 +23:56:19.29 AT 2026ivk 2026-04-07.91 18.97
09:57:07.898 +44:06:56.68 AT 2026ivj 2026-03-30.18 19.5868
11:56:46.937 +30:48:49.43 AT 2026ivi 2026-04-07.29 20.1063
12:16:21.919 +30:21:04.60 AT 2026ivh 2026-04-07.29 19.651
09:11:45.682 +30:03:32.51 AT 2026ivg 2026-04-04.17 19.5142
09:55:25.809 -27:42:27.02 AT 2026ivf 2026-04-08.21 18.51
09:46:07.094 +07:14:13.61 AT 2026ive 2026-04-08.15 19.9446
09:29:29.340 -01:21:08.51 AT 2026ivd 2026-04-05.15 19.4593
09:53:27.521 +16:01:50.20 AT 2026ivc 2026-04-07.17 20.1328
10:57:27.283 +18:19:29.99 AT 2026ivb 2026-04-07.87 19.71
12:50:08.105 +01:17:40.78 AT 2026iva 2026-04-07.89 19.96
10:38:31.370 -04:47:42.62 AT 2026iuz 2026-04-07.85 18.9
13:03:44.252 +20:35:06.20 AT 2026iuy 2026-04-06.96 19.7
13:53:33.216 -46:24:12.81 AT 2026iux 2026-04-07.63 19.83
-rw-r--r-- 1 apache apache 30K Apr 14 03:02 tns_transients_list.txt
