This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.1777-02.2246,2461130.6515,12.31,0.05,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
ATO J103.1777-02.2246 20260331.1515 12.31CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.0616-05.0067,2461130.6515,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.0616-05.0067 20260331.1515 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.4261-05.2596,2461130.6515,11.12,0.05,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
ATO J097.4261-05.2596 20260331.1515 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0653-02.3877,2461130.6515,11.67,0.05,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
ATO J106.0653-02.3877 20260331.1515 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.1449-04.3466,2461130.6515,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.1449-04.3466 20260331.1515 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111421128386749952,2461130.6515,11.51,0.05,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
Gaia DR3 3111421128386749952 20260331.1515 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109199054047735936,2461130.6515,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109199054047735936 20260331.1515 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8650-01.8472,2461130.6515,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8650-01.8472 20260331.1515 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1631+01.7787,2461130.6515,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1631+01.7787 20260331.1515 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101764396936908416,2461130.6515,11.31,0.05,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
Gaia DR3 3101764396936908416 20260331.1515 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107635033119937152,2461130.6515,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107635033119937152 20260331.1515 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4169-01.4407,2461130.6515,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4169-01.4407 20260331.1515 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053341183300774272,2461130.6515,11.01,0.05,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 3053341183300774272 20260331.1515 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.0216-02.7907,2461130.6515,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.0216-02.7907 20260331.1515 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0855 Mon,2461130.6515,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0855 Mon 20260331.1515 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108469734241394944,2461130.6515,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108469734241394944 20260331.1515 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0599-03.2490,2461130.6515,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0599-03.2490 20260331.1515 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4664-05.7173,2461130.6515,11.38,0.05,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
ATO J107.4664-05.7173 20260331.1515 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107692620041957376,2461130.6515,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107692620041957376 20260331.1515 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461130.6515,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260331.1515 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109310688836613632,2461130.6515,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109310688836613632 20260331.1515 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0653241-012719,2461130.6515,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0653241-012719 20260331.1515 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0855 Mon,2461130.6515,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0855 Mon 20260331.1515 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108641979610105088,2461130.6515,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108641979610105088 20260331.1515 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109408648450653696,2461130.6515,11.73,0.05,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 3109408648450653696 20260331.1515 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0957-05.1917,2461130.6515,11.59,0.05,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
ATO J103.0957-05.1917 20260331.1515 11.59CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0700298-000606,2461130.6515,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0700298-000606 20260331.1515 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HD 50209,2461130.6515,11.95,0.05,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
HD 50209 20260331.1515 11.95CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0247-02.8623,2461130.6515,12.04,0.05,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
ATO J105.0247-02.8623 20260331.1515 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461130.6515,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260331.1515 12.20CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070529-0200.2,2461130.6515,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070529-0200.2 20260331.1515 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DS Mon,2461130.6515,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DS Mon 20260331.1515 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12582051,2461130.6515,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12582051 20260331.1515 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AG Mon,2461130.6515,10.02,0.05,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
AG Mon 20260331.1515 10.02CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BM Mon,2461130.6515,11.05,0.05,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
BM Mon 20260331.1515 11.05CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0629023-003924,2461130.6515,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0629023-003924 20260331.1515 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461130.65222964 31.03.2026 03:39:02.641 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 6 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): 28655
Objects passed selection criteria: 28443
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 18167.5
Average stars matched: 17327 (95.3736 %)
Memory usage VmPeak: 133500 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Mon Mar 30 15:05:05 CDT 2026
VaST build number 1.0rc88-366-gda650e08
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-30)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 22:41:31 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461130.65222964 31.03.2026 03:39:02.641 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 107
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 37 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): 210104
Objects passed selection criteria: 209404
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 140716
Average stars matched: 132460 (94.1327 %)
Memory usage VmPeak: 2031900 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Mon Mar 30 15:05:05 CDT 2026
VaST build number 1.0rc88-366-gda650e08
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-30)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 22:46:09 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.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: 2461130.65069142
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits'
wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:41.070 -01:58:48.11
Angular distance between the image centers 0.03 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:42.874 -01:59:03.60
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:51:41.070 -01:58:48.11
Second-epoch second image center 06:51:42.874 -01:59:03.60
Angular distance between the image centers 0.00866 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.WcTAxH95PN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.IIMv116XLj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.648K7Dsyj8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits &> /tmp/tmp.DQYKG5s5tY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.4 pix fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
2.4 pix fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.1 mag. fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
13.2 mag. fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.5 (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.WcTAxH95PN (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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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...
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 16.11"
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...
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 16.01"
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.IIMv116XLj (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/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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...
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.00"
ERROR: the estimated accuracy of the plate solution seems unrealistically small!
Something is very wrong!
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.648K7Dsyj8 (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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=634, passed=7398
Got 7398 stars (including 6759 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 7398 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.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.DQYKG5s5tY (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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=556, passed=7046
Got 7046 stars (including 6482 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat
util/solve_plate_with_UCAC5 got 7046 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 926 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:41.070 -01:58:48.11
Angular distance between the image centers 0.03 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:42.874 -01:59:03.60
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:51:41.070 -01:58:48.11
Second-epoch second image center 06:51:42.874 -01:59:03.60
Angular distance between the image centers 0.00866 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.8IfZAcZKnD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.QDwLJLP9Hn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.cOgFZJtv3J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits &> /tmp/tmp.4s10FfLQW9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 82 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.3 pix fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
2.3 pix fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
12.4 mag. fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
12.4 mag. fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 11.9 (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.8IfZAcZKnD (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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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...
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 7.43"
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...
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 7.42"
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.QDwLJLP9Hn (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/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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...
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.00"
ERROR: the estimated accuracy of the plate solution seems unrealistically small!
Something is very wrong!
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cOgFZJtv3J (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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=4473, passed=67446
Got 67446 stars (including 62900 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 67446 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.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.4s10FfLQW9 (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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=4082, passed=64007
Got 64007 stars (including 59856 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat
util/solve_plate_with_UCAC5 got 64007 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-36-49_20.00sec_-15.00C_LIGHT_0027.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.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_2026-03-30_CI_Mon-02-Q2b1x1_223955_TTUQ2b1x1_20393_3aUtHvLV/wcs_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out285082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out121122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47993.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 46s
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: 23s
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Considering the candidate 285069_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285069_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285074_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285074_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:51:02.57 +01:07:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285082_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285082_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:04:36.81 -01:40:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.925 3109456094950953344 106.15260396703 -01.66850726094 12.9200 12.5571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285090_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285090_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:01:13.85 -03:36:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.780 3102603805347108864 105.30706796189 -03.61185024820 12.7881 12.0508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285091_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285091_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:29:27.82 -06:12:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.108 3103333223930303232 097.36575514434 -06.21048475434 11.6984 11.2008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285098_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285098_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:28:38.75 -05:29:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.928 3104136451535916032 097.16092228276 -05.49331653548 11.4771 10.9447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285101_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285101_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285104_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285104_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:29:06.09 -06:19:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 2.979 3007254771158500352 097.27478186336 -06.31744191355 11.5147 11.0763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285105_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285105_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:09:45.49 -03:50:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 3.135 3107648845734499072 107.43893066964 -03.84437200795 12.8237 12.0338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285109_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285109_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:43:54.04 -04:44:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 1.111 3103734167718005504 100.97527945473 -04.73540714355 12.0102 10.9461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285112_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285112_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:02:17.78 -05:08:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 5.101 3101407124380573056 105.57393999298 -05.14125681453 12.2840 11.1294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285113_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285113_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285116_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285116_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285118_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285118_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285124_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285124_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285125_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285125_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285127_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285127_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:07:33.48 -02:48:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 2.939 3108018247278107904 106.88869129625 -02.80810312876 12.3336 11.6435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285131_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285131_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285133_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285133_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285136_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285136_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285137_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285137_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:51:44.53 +00:30:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285139_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285139_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285142_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285142_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
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Considering the candidate 285146_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285146_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285147_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285147_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:58:26.77 -00:54:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 3.360 3112253325548814208 104.61066330762 -00.91453798124 11.7888 10.7799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285150_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285150_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:14:24.43 +01:15:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.068 3111803861510882688 108.60133408623 +01.26012490561 11.9672 11.5588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285151_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 285151_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285154_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 285154_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:07:49.56 -05:43:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 1.202 3053313317552123136 106.95621729906 -05.71917980454 11.4603 10.8192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 287507_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 287507_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:50:40.26 -00:32:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288868_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 288868_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:51:37.31 +00:26:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 1.638 3113576308614129408 102.90501560737 +00.44942258340 11.7443 11.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289464_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 289464_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:51:39.79 +00:25:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289539_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 289539_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289820_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 289820_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:02:55.48 -04:15:44.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289941_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 289941_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290018_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 290018_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290381_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 290381_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290993_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 290993_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:03:00.91 -04:14:53.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291078_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 291078_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:54:00.58 -04:24:09.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291205_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 291205_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:02:11.36 -06:02:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291233_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 291233_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:40:30.75 -01:04:43.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291462_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 291462_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:15:39.16 -01:52:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 2.092 3108327343185110784 108.91263520722 -01.87187473211 12.5693 12.4702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291640_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 291640_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:50:41.70 -00:33:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291716_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 291716_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:06:26.26 -03:07:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 4.047 3107980176688510592 106.60829315764 -03.13101077576 12.2605 11.5350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291895_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 291895_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:52:25.57 -05:17:26.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292057_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 292057_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292084_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 292084_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:40:37.79 +00:43:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 1.010 3119794424826044928 100.15717896773 +00.71691830212 11.9547 11.2893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292335_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 292335_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292349_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 292349_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:05:30.88 -00:46:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 5.532 3109670744533855616 106.37713108502 -00.76974192019 12.6635 11.7610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292458_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 292458_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:03:58.94 -05:19:54.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292481_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 292481_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:42:50.67 -04:09:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 2.368 3105326780250358016 100.71103536226 -04.15301287620 11.9882 11.2872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292649_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 292649_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292700_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 292700_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:03:11.96 -02:15:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.492 3108852222548310656 105.79942401951 -02.25617766869 12.3669 11.3998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292772_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 292772_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:07:16.77 -04:03:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 2.367 3107593870154767744 106.82014353931 -04.06254484292 12.5758 11.6556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292921_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 292921_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292927_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 292927_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293076_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 293076_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293240_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 293240_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293252_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 293252_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293316_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 293316_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:15:37.65 -01:51:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.045 3108327416208346496 108.90715063336 -01.86520245758 12.5792 11.7354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293404_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 293404_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:12:38.98 -00:39:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 0.871 3110941363360070784 108.16242662314 -00.66454720605 12.5974 11.8411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293580_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 293580_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:02:22.07 -03:19:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 5.799 3108623008734853504 105.59046160933 -03.32654619758 12.1808 10.8341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294240_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 294240_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294351_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 294351_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:01:52.80 -01:19:04.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294424_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 294424_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:02:39.78 -04:37:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.091 3101534633371804672 105.66529147356 -04.63116397367 12.8393 12.0875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294552_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 294552_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295422_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 295422_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:50:44.58 -00:31:38.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295485_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 295485_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295667_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 295667_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:56:49.29 -03:40:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295921_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 295921_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:06:52.72 -00:27:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 5.011 3109706135063598592 106.71842488065 -00.45571211931 13.1534 12.3288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296435_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 296435_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:54:30.24 -04:07:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296469_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 296469_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 07:01:22.56 -03:06:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.476 3108642426286693376 105.34338227084 -03.10135969197 12.9086 11.8972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296488_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 296488_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182305_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 182305_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:27:15.79 -00:16:34.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131156_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 131156_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47889_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 47889_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47993_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 47993_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57802_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 57802_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:45:42.45 -04:56:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 121122_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 199360_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169859_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
Preparing report for the candidate 169859_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49190_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 49190_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:35:46.84 -05:22:34.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63748_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028
The candidate 63748_fd_Mon-02-Q2b1x1_2026-03-30_22-39-02_20.00sec_-15.00C_LIGHT_0028 did not pass the final checks
**** FOUND 06:27:57.74 -04:45:41.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 72s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:13.74 -02:21:31.2
07:05:28.62 -02:00:08.8
06:29:02.82 -00:39:21.1
07:08:45.41 +00:41:47.1
06:52:42.59 -02:13:37.0
06:56:14.06 -05:00:25.7
06:29:42.99 -05:15:39.7
07:04:15.83 -02:22:59.5
06:32:34.38 -04:20:54.6
07:12:40.30 +01:01:20.6
07:07:26.06 -02:04:12.5
07:07:26.06 -01:50:46.4
07:08:35.72 +01:46:43.8
07:03:56.34 -04:08:26.8
07:10:59.23 -03:55:09.6
07:09:43.11 -01:26:31.6
07:08:38.16 -05:29:39.2
07:16:02.31 -02:48:05.8
06:51:49.67 +00:28:03.5
07:13:11.52 -02:19:21.2
07:04:10.76 -03:14:38.1
07:09:52.41 -05:43:16.6
07:11:21.71 -03:21:40.5
07:05:52.46 -01:02:31.4
07:07:09.18 -01:18:58.6
06:53:24.26 -01:27:19.6
06:51:50.18 +00:28:20.3
07:01:23.25 -03:07:23.1
07:08:25.04 -01:06:46.1
06:52:20.52 -05:11:35.3
07:00:27.50 -00:06:04.7
06:52:11.88 -00:18:24.5
07:00:06.68 -02:51:35.6
06:54:51.42 -01:22:17.6
06:44:47.63 -05:17:45.5
06:51:26.47 -05:15:24.3
########### Completed Mon-02-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 ####
06:52:42.59 -02:13:37.0
06:56:14.06 -05:00:25.7
06:29:42.99 -05:15:39.7
07:04:15.83 -02:22:59.5
06:32:34.38 -04:20:54.6
07:12:40.30 +01:01:20.6
07:07:26.06 -02:04:12.5
07:07:26.06 -01:50:46.4
07:08:35.72 +01:46:43.8
07:03:56.34 -04:08:26.8
07:10:59.23 -03:55:09.6
07:09:43.11 -01:26:31.6
07:08:38.16 -05:29:39.2
07:16:02.31 -02:48:05.8
06:51:49.67 +00:28:03.5
07:13:11.52 -02:19:21.2
07:04:10.76 -03:14:38.1
07:09:52.41 -05:43:16.6
07:11:21.71 -03:21:40.5
07:05:52.46 -01:02:31.4
07:07:09.18 -01:18:58.6
06:53:24.26 -01:27:19.6
06:51:50.18 +00:28:20.3
07:01:23.25 -03:07:23.1
07:08:25.04 -01:06:46.1
06:52:20.52 -05:11:35.3
07:00:27.50 -00:06:04.7
06:52:11.88 -00:18:24.5
07:00:06.68 -02:51:35.6
06:54:51.42 -01:22:17.6
07:05:28.62 -02:00:08.8
06:44:47.63 -05:17:45.5
06:51:26.47 -05:15:24.3
07:09:13.74 -02:21:31.2
07:08:45.41 +00:41:47.1
06:29:02.82 -00:39:21.1
###################################################################################
06:52:42.59 -02:13:37.0 -- not an asteroid (will add it to exclusion list)
06:56:14.06 -05:00:25.7 -- not an asteroid (will add it to exclusion list)
06:29:42.99 -05:15:39.7 -- not an asteroid (will add it to exclusion list)
07:04:15.83 -02:22:59.5 -- not an asteroid (will add it to exclusion list)
06:32:34.38 -04:20:54.6 -- not an asteroid (will add it to exclusion list)
07:12:40.30 +01:01:20.6 -- not an asteroid (will add it to exclusion list)
07:07:26.06 -02:04:12.5 -- not an asteroid (will add it to exclusion list)
07:07:26.06 -01:50:46.4 -- not an asteroid (will add it to exclusion list)
07:08:35.72 +01:46:43.8 -- not an asteroid (will add it to exclusion list)
07:03:56.34 -04:08:26.8 -- not an asteroid (will add it to exclusion list)
07:10:59.23 -03:55:09.6 -- not an asteroid (will add it to exclusion list)
07:09:43.11 -01:26:31.6 -- not an asteroid (will add it to exclusion list)
07:08:38.16 -05:29:39.2 -- not an asteroid (will add it to exclusion list)
07:16:02.31 -02:48:05.8 -- not an asteroid (will add it to exclusion list)
06:51:49.67 +00:28:03.5 -- not an asteroid (will add it to exclusion list)
07:13:11.52 -02:19:21.2 -- not an asteroid (will add it to exclusion list)
07:04:10.76 -03:14:38.1 -- not an asteroid (will add it to exclusion list)
07:09:52.41 -05:43:16.6 -- not an asteroid (will add it to exclusion list)
07:11:21.71 -03:21:40.5 -- not an asteroid (will add it to exclusion list)
07:05:52.46 -01:02:31.4 -- not an asteroid (will add it to exclusion list)
07:07:09.18 -01:18:58.6 -- not an asteroid (will add it to exclusion list)
06:53:24.26 -01:27:19.6 -- not an asteroid (will add it to exclusion list)
06:51:50.18 +00:28:20.3 -- not an asteroid (will add it to exclusion list)
07:01:23.25 -03:07:23.1 -- not an asteroid (will add it to exclusion list)
07:08:25.04 -01:06:46.1 -- not an asteroid (will add it to exclusion list)
06:52:20.52 -05:11:35.3 -- not an asteroid (will add it to exclusion list)
07:00:27.50 -00:06:04.7 -- not an asteroid (will add it to exclusion list)
06:52:11.88 -00:18:24.5 -- not an asteroid (will add it to exclusion list)
07:00:06.68 -02:51:35.6 -- not an asteroid (will add it to exclusion list)
06:54:51.42 -01:22:17.6 -- not an asteroid (will add it to exclusion list)
07:05:28.62 -02:00:08.8 -- not an asteroid (will add it to exclusion list)
06:44:47.63 -05:17:45.5 -- not an asteroid (will add it to exclusion list)
06:51:26.47 -05:15:24.3 -- not an asteroid (will add it to exclusion list)
07:09:13.74 -02:21:31.2 -- not an asteroid (will add it to exclusion list)
07:08:45.41 +00:41:47.1 -- not an asteroid (will add it to exclusion list)
06:29:02.82 -00:39:21.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:29:02.82 -00:39:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:42.99 -05:15:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:34.38 -04:20:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:47.63 -05:17:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:26.47 -05:15:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:49.67 +00:28:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:50.18 +00:28:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:11.88 -00:18:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:20.52 -05:11:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:42.59 -02:13:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:24.26 -01:27:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:51.42 -01:22:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:14.06 -05:00:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:06.68 -02:51:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:27.50 -00:06:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:23.25 -03:07:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:56.34 -04:08:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.76 -03:14:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:15.83 -02:22:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:28.62 -02:00:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:52.46 -01:02:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:09.18 -01:18:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:26.06 -01:50:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:26.06 -02:04:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:25.04 -01:06:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:35.72 +01:46:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:38.16 -05:29:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:45.41 +00:41:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.74 -02:21:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:43.11 -01:26:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:52.41 -05:43:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:59.23 -03:55:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:21.71 -03:21:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:40.30 +01:01:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:11.52 -02:19:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:02.31 -02:48:05.8 -- 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)
06:29:02.82 -00:39:21.1 -- a known variable star
06:29:42.99 -05:15:39.7 -- not a known variable star
06:32:34.38 -04:20:54.6 -- not a known variable star
06:44:47.63 -05:17:45.5 -- a known variable star
06:51:26.47 -05:15:24.3 -- a known variable star
06:51:49.67 +00:28:03.5 -- a known variable star
06:51:50.18 +00:28:20.3 -- a known variable star
06:52:11.88 -00:18:24.5 -- not a known variable star
06:52:20.52 -05:11:35.3 -- not a known variable star
06:52:42.59 -02:13:37.0 -- not a known variable star
06:53:24.26 -01:27:19.6 -- a known variable star
06:54:51.42 -01:22:17.6 -- not a known variable star
06:56:14.06 -05:00:25.7 -- not a known variable star
07:00:06.68 -02:51:35.6 -- not a known variable star
07:00:27.50 -00:06:04.7 -- a known variable star
07:01:23.25 -03:07:23.1 -- a known variable star
07:03:56.34 -04:08:26.8 -- a known variable star
07:04:10.76 -03:14:38.1 -- not a known variable star
07:04:15.83 -02:22:59.5 -- not a known variable star
07:05:28.62 -02:00:08.8 -- a known variable star
07:05:52.46 -01:02:31.4 -- not a known variable star
07:07:09.18 -01:18:58.6 -- a known variable star
07:07:26.06 -01:50:46.4 -- not a known variable star
07:07:26.06 -02:04:12.5 -- a known variable star
07:08:25.04 -01:06:46.1 -- not a known variable star
07:08:35.72 +01:46:43.8 -- not a known variable star
07:08:38.16 -05:29:39.2 -- not a known variable star
07:08:45.41 +00:41:47.1 -- a known variable star
07:09:13.74 -02:21:31.2 -- a known variable star
07:09:43.11 -01:26:31.6 -- not a known variable star
07:09:52.41 -05:43:16.6 -- not a known variable star
07:10:59.23 -03:55:09.6 -- not a known variable star
07:11:21.71 -03:21:40.5 -- a known variable star
07:12:40.30 +01:01:20.6 -- not a known variable star
07:13:11.52 -02:19:21.2 -- not a known variable star
07:16:02.31 -02:48:05.8 -- not a known variable star
Found 21 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
36 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 ####
06:29:02.82 -00:39:21.1
06:29:42.99 -05:15:39.7
06:32:34.38 -04:20:54.6
06:44:47.63 -05:17:45.5
06:51:26.47 -05:15:24.3
06:51:49.67 +00:28:03.5
06:51:50.18 +00:28:20.3
06:52:11.88 -00:18:24.5
06:52:20.52 -05:11:35.3
06:52:42.59 -02:13:37.0
06:53:24.26 -01:27:19.6
06:54:51.42 -01:22:17.6
06:56:14.06 -05:00:25.7
07:00:06.68 -02:51:35.6
07:00:27.50 -00:06:04.7
07:01:23.25 -03:07:23.1
07:03:56.34 -04:08:26.8
07:04:10.76 -03:14:38.1
07:04:15.83 -02:22:59.5
07:05:28.62 -02:00:08.8
07:05:52.46 -01:02:31.4
07:07:09.18 -01:18:58.6
07:07:26.06 -01:50:46.4
07:07:26.06 -02:04:12.5
07:08:25.04 -01:06:46.1
07:08:35.72 +01:46:43.8
07:08:38.16 -05:29:39.2
07:08:45.41 +00:41:47.1
07:09:13.74 -02:21:31.2
07:09:43.11 -01:26:31.6
07:09:52.41 -05:43:16.6
07:10:59.23 -03:55:09.6
07:11:21.71 -03:21:40.5
07:12:40.30 +01:01:20.6
07:13:11.52 -02:19:21.2
07:16:02.31 -02:48:05.8
07:04:36.81 -01:40:05.7
07:01:13.85 -03:36:41.1
06:29:27.82 -06:12:36.8
06:28:38.75 -05:29:36.1
06:29:06.09 -06:19:00.7
07:09:45.49 -03:50:37.5
06:43:54.04 -04:44:08.5
07:02:17.78 -05:08:33.6
07:07:33.48 -02:48:29.6
06:58:26.77 -00:54:51.2
07:14:24.43 +01:15:37.7
07:07:49.56 -05:43:08.4
06:51:37.31 +00:26:58.3
07:15:39.16 -01:52:17.9
07:06:26.26 -03:07:51.9
06:40:37.79 +00:43:01.0
07:05:30.88 -00:46:11.3
06:42:50.67 -04:09:08.5
07:03:11.96 -02:15:22.0
07:07:16.77 -04:03:43.0
07:15:37.65 -01:51:54.4
07:12:38.98 -00:39:51.5
07:02:22.07 -03:19:33.4
07:02:39.78 -04:37:50.9
07:06:52.72 -00:27:18.3
07:01:22.56 -03:06:03.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461130.65069142 -observatory V36
22:57:44.92 -07:53:58.1 Mercury (0.5mag)
01:53:11.48 +11:06:05.0 Venus (-3.9mag)
23:32:34.61 -04:06:07.8 Mars (1.2mag)
07:06:50.65 +22:55:12.0 Jupiter (-2.2mag)
00:22:00.07 +00:03:41.7 Saturn (0.9mag)
03:44:36.44 +19:37:26.2 Uranus (5.8mag)
00:08:41.99 -00:28:58.0 Neptune (7.8mag)
20:32:49.74 -22:52:45.9 Pluto (14.5mag)
11:13:06.91 +03:52:53.4 Moon (-12.1mag)
-rw-r--r-- 1 apache apache 362 Mar 30 22:41 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461130.65069142:
07:06:50.60 +22:55:14.7 Io (5.7mag)
07:06:44.60 +22:55:20.9 Europa (5.8mag)
07:07:04.05 +22:54:51.9 Ganymede (5.2mag)
07:07:26.15 +22:54:01.6 Callisto (6.5mag)
07:10:43.69 +22:50:59.3 Himalia (15.2mag)
07:06:48.54 +22:55:18.2 Thebe (16.1mag)
07:10:32.45 +23:18:08.2 Elara (17.2mag)
07:04:38.96 +23:43:30.9 Pasiphae (17.3mag)
07:15:28.91 +22:51:19.2 Carme (18.4mag)
00:22:00.41 +00:04:06.2 Titan (8.8mag)
00:22:04.69 +00:03:50.6 Rhea (10.1mag)
00:22:14.15 +00:05:46.0 Iapetus (11.5mag)
00:21:50.12 +00:04:02.5 Hyperion (14.8mag)
00:23:48.32 +00:14:05.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 30 22:41 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461130.65069142:
14:08:18.64 -02:18:33.2 JWST
11:09:41.51 +45:36:45.7 Chandra
07:52:03.48 -33:29:50.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 30 22:41 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461130.65069142 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:43:15.33 -27:55:52.1 14.0mag P/2010 H2 (Vales)
04:56:26.10 -70:28:04.8 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:41.33 +31:20:37.6 17.1mag C/2017 K2 (PANSTARRS)
17:30:46.34 +08:38:06.6 17.6mag C/2021 G2 (ATLAS)
23:05:19.56 +28:40:48.2 17.0mag C/2022 E2 (ATLAS)
04:11:17.45 +25:35:22.3 15.8mag C/2022 N2 (PANSTARRS)
09:01:29.95 +31:46:41.4 16.1mag C/2022 QE78 (ATLAS)
08:29:46.28 -01:56:16.4 17.2mag C/2022 R6 (PANSTARRS)
18:56:14.20 +17:10:11.9 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:51.55 -11:44:16.0 17.6mag P/2023 B1 (PANSTARRS)
09:16:45.07 -14:32:37.3 17.5mag C/2023 F3 (ATLAS)
21:35:55.78 +62:05:14.4 17.4mag C/2023 H5 (Lemmon)
19:29:37.05 -03:33:49.6 14.3mag C/2023 R1 (PANSTARRS)
21:42:26.53 +83:53:29.5 17.8mag C/2023 X2 (Lemmon)
06:13:50.33 +63:39:06.0 17.0mag C/2024 A1 (ATLAS)
04:35:51.21 +11:37:13.4 9.9mag C/2024 E1 (Wierzchos)
16:28:08.89 +03:47:21.6 17.4mag C/2024 G6 (ATLAS)
20:15:01.90 +11:10:06.6 14.8mag C/2024 J3 (ATLAS)
03:12:42.70 -24:54:55.5 16.4mag C/2024 T5 (ATLAS)
05:04:10.80 +49:31:35.9 17.6mag C/2025 J1 (Borisov)
14:41:54.63 +30:40:33.7 14.6mag C/2025 L1 (ATLAS)
03:01:49.10 -23:54:40.0 17.7mag C/2025 Q3 (ATLAS)
22:42:15.65 +19:39:19.1 11.1mag C/2025 R3 (PANSTARRS)
13:00:58.97 +01:59:30.0 17.5mag C/2025 Y1 (ATLAS)
01:34:49.61 +00:38:23.8 10.5mag C/2026 A1 (MAPS)
23:12:04.24 +33:49:34.4 14.1mag C/2026 B2 (Sun-Gao)
18:11:57.80 -10:29:08.5 12.7mag 10P/Tempel
15:19:23.90 +04:33:01.3 12.6mag 24P/Schaumasse
11:07:56.07 -02:05:22.7 15.7mag 29P/Schwassmann-Wachmann
17:52:44.62 -10:14:27.9 17.6mag 40P/Vaisala
10:40:39.80 -05:31:58.5 16.6mag 43P/Wolf-Harrington
01:24:19.05 +14:44:04.0 17.1mag 47P/Ashbrook-Jackson
06:43:25.90 +40:19:03.1 17.1mag 63P/Wild
23:08:12.44 -13:25:17.7 15.7mag 65P/Gunn
03:22:37.02 +15:25:29.6 15.8mag 76P/West-Kohoutek-Ikemura
00:31:03.13 +05:04:38.4 14.5mag 78P/Gehrels
22:12:58.73 -13:59:53.2 14.5mag 88P/Howell
01:26:59.02 +16:12:56.1 15.2mag 93P/Lovas
04:26:37.08 +31:21:05.0 16.4mag 123P/West-Hartley
08:12:56.24 +45:40:18.8 16.2mag 124P/Mrkos
02:09:10.31 +12:33:14.7 16.4mag 128P/Shoemaker-Holt
02:16:44.38 +12:26:50.8 17.4mag 131P/Mueller
00:06:29.18 +07:12:05.4 11.8mag 141P/Machholz
00:16:43.63 -00:59:46.1 11.9mag 141P-A/Machholz
23:10:59.07 -04:14:27.2 14.8mag 141P-D/Machholz
00:18:26.71 -09:21:49.8 15.3mag 162P/SidingSpring
10:33:23.91 +31:48:22.2 17.7mag 164P/Christensen
06:07:30.31 +24:38:20.3 17.7mag 198P/ODAS
15:18:43.42 -01:59:05.2 17.2mag 210P/Christensen
20:48:45.75 -15:15:43.3 17.3mag 218P/LINEAR
17:08:34.76 -15:43:08.5 16.2mag 235P/LINEAR
05:01:17.32 +33:13:47.6 16.5mag 240P/NEAT
07:32:09.94 -07:02:05.8 17.6mag 242P/Spahr
15:47:21.09 +05:51:48.6 17.6mag 391P/Kowalski
07:29:27.14 +21:15:07.5 17.6mag 450P/LONEOS
05:13:45.64 +45:58:36.0 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 30 22:41 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 30 22:41 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
03:17:02.234 +03:38:58.77 AT 2026hdl 2026-03-24.12 18.7238
03:50:10.370 +20:05:23.90 AT 2026hdk 2026-03-25.13 19.6517
04:20:08.576 -08:40:40.60 AT 2026hdj 2026-03-24.14 18.4123
03:27:48.232 +40:02:03.56 SN 2026hdi 2026-03-24.13 18.9792
05:57:07.261 +53:40:05.12 AT 2026hdh 2026-03-19.16 20.4416
09:50:38.793 +12:38:39.43 AT 2026hdg 2026-03-23.26 20.3707
10:39:04.665 +24:32:28.39 AT 2026hdf 2026-03-19.32 20.7192
10:47:24.765 +23:23:02.26 AT 2026hde 2026-03-15.37 21.0555
07:08:13.650 +62:41:32.00 AT 2026hdd 2026-03-19.16 20.8135
13:22:29.360 -15:55:17.10 AT 2026hdc 2026-03-24.27 19.8
03:39:08.753 -28:16:13.12 AT 2026hdb 2026-03-10.04 23.486
03:33:23.017 -29:34:24.74 AT 2026hda 2026-03-10.14 22.885
03:35:17.945 -29:23:38.62 AT 2026hcz 2026-03-07.04 22.496
08:51:57.897 -19:15:16.03 AT 2026hcy 2026-03-14.40 20.53
09:59:55.163 +00:32:15.02 AT 2026hcx 2026-03-20.48 20.28
09:11:21.221 -68:52:07.67 AT 2026hcw 2026-03-24.41 19.91
12:46:27.910 -19:20:04.06 AT 2026hcv 2026-03-20.51 20.34
12:58:10.446 -07:08:06.36 AT 2026hcu 2026-03-22.53 20.08
04:48:04.523 -25:13:50.64 AT 2026hct 2026-03-21.76 18.866
08:01:00.881 +14:50:56.31 AT 2026hcs 2026-03-21.14 21.0409
-rw-r--r-- 1 apache apache 30K Mar 30 22:41 tns_transients_list.txt
