This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1401148074327914112,2461146.9325,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1401148074327914112 20260416.4325 12.49CV 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!
TCP 2026 04 16.4325* 15 50 19.15 +46 30 00.7 12.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1398035150750619520,2461146.9325,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1398035150750619520 20260416.4325 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 15 57 30.36 +45 40 01.9 12.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1396958007312843520,2461146.9325,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1396958007312843520 20260416.4325 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 16 04 38.42 +44 56 53.9 15.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J241.1631+44.9520,2461146.9325,14.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J241.1631+44.9520 20260416.4325 14.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2889406,2461146.9325,14.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
DocumentRef: VOTx2889406 20260416.4325 14.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 16 10 58.57 +42 51 21.0 14.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.38CV 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!
TCP 2026 04 16.4325* 16 09 57.95 +41 28 40.1 14.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1402819061419589376,2461146.9325,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1402819061419589376 20260416.4325 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1592056312617779328,2461146.9325,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1592056312617779328 20260416.4325 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 15 59 55.00 +49 49 20.2 14.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3145591,2461146.9325,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
DocumentRef: VOTx3145591 20260416.4325 14.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1402665885706537728,2461146.9325,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1402665885706537728 20260416.4325 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 16 06 45.80 +49 22 27.4 14.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 16 24 40.05 +49 45 56.9 14.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 15 59 52.90 +49 49 19.1 14.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3167231,2461146.9325,14.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
DocumentRef: VOTx3167231 20260416.4325 14.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J226.6189+46.3442,2461146.9325,14.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J226.6189+46.3442 20260416.4325 14.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4325* 16 25 00.18 +49 30 07.3 15.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,15.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 15.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9325,14.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260416.4325 14.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J223.1758+46.1421,2461146.9325,14.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J223.1758+46.1421 20260416.4325 14.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.95385653 22.03.2026 10:53:23.204 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
First image: 2461121.95385653 22.03.2026 10:53:23.204 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Last image: 2461146.93283980 16.04.2026 10:23:07.359 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8756
Objects passed selection criteria: 8752
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 8458
Average stars matched: 8215 (97.127 %)
Memory usage VmPeak: 114064 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 06:19:44 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: 2461121.95385653 22.03.2026 10:53:23.204 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
First image: 2461121.95385653 22.03.2026 10:53:23.204 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Last image: 2461146.93283980 16.04.2026 10:23:07.359 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 85
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.16
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: 32 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): 48018
Objects passed selection criteria: 47899
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 46542
Average stars matched: 44686.8 (96.0138 %)
Memory usage VmPeak: 146660 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 06:23:58 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
SExtractor catalog cache: saved Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat to cache
SExtractor catalog cache: saved Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.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/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.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: 2461146.93209678
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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits exists and is non-empty
Saving wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits to local_wcs_cache/
'wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits' -> 'local_wcs_cache/wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits'
wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits exists and is non-empty
Saving wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits to local_wcs_cache/
'wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits' -> 'local_wcs_cache/wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits'
wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits exists and is non-empty
Saving wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits to local_wcs_cache/
'wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits' -> 'local_wcs_cache/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits'
wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits exists and is non-empty
Saving wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits to local_wcs_cache/
'wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits' -> 'local_wcs_cache/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits (1st reference image)
verification OK: wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:36:01.910 +45:59:31.44 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits (1st new image)
verification OK: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:36:10.923 +45:59:10.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:36:01.910 +45:59:31.44
Second-epoch image center 15:36:10.923 +45:59:10.42
Angular distance between the image centers 0.0267 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits (2nd new image)
verification OK: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:36:08.685 +45:58:36.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:36:01.910 +45:59:31.44
Second-epoch image center 15:36:08.685 +45:58:36.12
Angular distance between the image centers 0.0249 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 15:36:10.923 +45:59:10.42
Second-epoch second image center 15:36:08.685 +45:58:36.12
Angular distance between the image centers 0.01152 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/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits &> /tmp/tmp.Rp3qanquXK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits &> /tmp/tmp.GgBPAi0yeM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits &> /tmp/tmp.2AmPJza0Ik
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits &> /tmp/tmp.kdCQu08H54
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits and wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits and wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
Found non-empty wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits and wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
The reference image (wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits) and catalog (wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat) found
'wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat' -> 'wcsmag.cat'
Read 8468 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.0463 to 246.6904 deg, Dec +39.9538 to +51.3474 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 222.0463 to 246.6904 deg, Dec 39.9538 to 51.3474 deg
Loaded 5643 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): 3999 out of 4196 total matches.
Matched with Tycho-2 4196 out of 8468 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.954301
a=0.000000 b=1.000000 c=22.954301
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
2.0 pix Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
2.1 pix fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
2.1 pix fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Limiting magnitude estimates:
15.6 mag. Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
15.5 mag. Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
15.5 mag. fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
15.5 mag. fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 12.5 (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.Rp3qanquXK (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits' -> 'wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
WCS-calibrated image found: wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Checking if the catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
WCS catalog name: wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=531, passed=8468
Got 8468 stars (including 7920 good ones) from the SExtractor catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
util/solve_plate_with_UCAC5 got 8468 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 8331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 8332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 983 matched stars entering correct_measured_positions(), 8332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 983 stars left (next iteration limit 1081)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits -region wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.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.GgBPAi0yeM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits' -> 'wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
WCS-calibrated image found: wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
Checking if the catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
WCS catalog name: wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=548, passed=8538
Got 8538 stars (including 7979 good ones) from the SExtractor catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat
util/solve_plate_with_UCAC5 got 8538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 8391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 8390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 8390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits -region wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.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.2AmPJza0Ik (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Checking if the catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
WCS catalog name: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=503, passed=8495
Got 8495 stars (including 7978 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat
util/solve_plate_with_UCAC5 got 8495 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 8335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 8335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 8335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits -region wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.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.kdCQu08H54 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Checking if the catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
WCS catalog name: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=498, passed=8540
Got 8540 stars (including 8033 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat
util/solve_plate_with_UCAC5 got 8540 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 8421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 8421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 8421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits -region wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits'
Saving fully-calibrated image wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits'
Saving fully-calibrated image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits'
Saving fully-calibrated image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits'
Preparing the HTML report for the field Boo-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20527.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 178s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20452_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 20452_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 15:33:25.97 +42:45:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20519_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 20519_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 16:10:06.19 +43:36:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20521_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 20521_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20524_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 20524_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20527_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 20527_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 181s
Prepared the HTML report for the field Boo-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
15:38:04.43 +47:26:30.0
15:50:19.15 +46:30:00.7
15:57:30.36 +45:40:01.9
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
SExtractor catalog cache: saved Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat to cache
SExtractor catalog cache: saved Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Creating symlink local_wcs_cache/wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits exists and is non-empty
wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits exists and is non-empty
wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits exists and is non-empty
wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits (1st reference image)
verification OK: wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:36:01.910 +45:59:31.44 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits (1st new image)
verification OK: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:36:10.923 +45:59:10.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:36:01.910 +45:59:31.44
Second-epoch image center 15:36:10.923 +45:59:10.42
Angular distance between the image centers 0.0267 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits (2nd new image)
verification OK: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:36:08.685 +45:58:36.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:36:01.910 +45:59:31.44
Second-epoch image center 15:36:08.685 +45:58:36.12
Angular distance between the image centers 0.0249 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 15:36:10.923 +45:59:10.42
Second-epoch second image center 15:36:08.685 +45:58:36.12
Angular distance between the image centers 0.01152 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/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits &> /tmp/tmp.lmDxN4pYir
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits &> /tmp/tmp.LEpunZlb9H
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits &> /tmp/tmp.3zMytGmK8k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits &> /tmp/tmp.oNdDD169tp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits and wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits and wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
Found non-empty wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits and wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
The reference image (wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits) and catalog (wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat) found
'wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat' -> 'wcsmag.cat'
Read 47129 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.9937 to 246.7193 deg, Dec +39.9075 to +51.3493 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 221.9937 to 246.7193 deg, Dec 39.9075 to 51.3493 deg
Loaded 5685 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): 3779 out of 4211 total matches.
Matched with Tycho-2 4211 out of 47129 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.852762
a=0.000000 b=1.000000 c=22.852762
From vast_summary.log: estimated ref. image limiting mag.: -7.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.69
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.69
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 27 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
1.9 pix Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
2.0 pix fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
2.0 pix fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Limiting magnitude estimates:
15.7 mag. Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
15.7 mag. Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
15.7 mag. fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
15.7 mag. fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
All-image limiting magnitude estimate: 15.7 (SNR ) 14.9 (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.lmDxN4pYir (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits' -> 'wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
WCS-calibrated image found: wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Checking if the catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
WCS catalog name: wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2028, passed=47112
Got 47112 stars (including 45008 good ones) from the SExtractor catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat
util/solve_plate_with_UCAC5 got 47112 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 46448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 46447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 46447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits -region wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.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.LEpunZlb9H (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits' -> 'wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
WCS-calibrated image found: wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
Checking if the catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat corresponding to the image wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
WCS catalog name: wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2011, passed=46787
Got 46787 stars (including 44710 good ones) from the SExtractor catalog wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat
util/solve_plate_with_UCAC5 got 46787 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 46248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 46246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 46246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits -region wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.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.3zMytGmK8k (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Checking if the catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
WCS catalog name: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2060, passed=46804
Got 46804 stars (including 44653 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat
util/solve_plate_with_UCAC5 got 46804 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 46018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 46018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 46018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits -region wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.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.oNdDD169tp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Checking if the catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat corresponding to the image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
WCS catalog name: wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=2039, passed=46585
Got 46585 stars (including 44470 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat
util/solve_plate_with_UCAC5 got 46585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 45826 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 45826 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 45825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits -region wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.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_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_Boo-03-Q1b1x1_2026-03-22_05-53-23_20.00sec_-15.00C_LIGHT_0347.fits
Saving fully-calibrated image wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_Boo-03-Q1b1x1_2026-03-22_05-54-09_20.00sec_-15.00C_LIGHT_0348.fits
Saving fully-calibrated image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-22-03_20.00sec_-4.90C_LIGHTs_0350.fits
Saving fully-calibrated image wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Boo-03-Q1b1x1_052401_TTUQ1b1x1_9923_67Jdw6Zb/wcs_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351.fits
Preparing the HTML report for the field Boo-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53991.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53914.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 564s
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: 27s
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Considering the candidate 53244_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53244_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53245_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53245_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53246_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53246_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53250_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53250_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53252_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53252_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53253_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53253_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53256_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53256_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53258_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53258_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53261_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 53261_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 14:59:39.75 +50:11:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53263_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53263_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53265_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 53265_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 14:59:46.67 +44:07:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53270_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 53270_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 15:00:40.02 +47:16:07.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53358_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53358_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53505_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53505_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53622_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53622_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53632_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53632_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53681_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53681_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53822_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53822_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53832_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53832_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53870_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53870_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53889_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 53889_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 15:01:13.62 +43:32:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53890_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53890_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53909_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53909_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53914_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
Preparing report for the candidate 53914_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
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Considering the candidate 53923_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 53923_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 16:25:34.40 +49:28:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.258 1411312307708375040 246.39342849768 +49.48135266784 14.7007 14.0440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53938_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 53938_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 15:51:18.69 +43:58:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.190 1396751234703296512 237.82747698472 +43.96844641920 14.9137 14.4408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53991_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351
The candidate 53991_fd_Boo-03-Q1b1x1_2026-04-16_05-23-07_20.00sec_-4.90C_LIGHTs_0351 did not pass the final checks
**** FOUND 15:35:00.21 +43:08:48.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 594s
Prepared the HTML report for the field Boo-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
15:38:04.43 +47:26:30.0
15:50:19.15 +46:30:00.7
15:57:30.36 +45:40:01.9
15:18:42.10 +47:33:03.4
16:04:38.42 +44:56:53.9
15:23:30.50 +47:40:32.7
14:56:50.29 +42:16:32.0
16:10:58.57 +42:51:21.0
15:20:10.25 +48:11:31.1
14:55:38.28 +45:28:54.1
15:31:13.64 +42:52:39.7
16:09:57.95 +41:28:40.1
15:38:19.33 +50:20:21.6
15:00:09.01 +48:49:44.1
15:59:55.00 +49:49:20.2
15:34:18.15 +49:29:52.0
16:06:45.80 +49:22:27.4
16:24:40.05 +49:45:56.9
15:59:52.90 +49:49:19.1
15:06:28.60 +46:20:39.7
16:25:00.18 +49:30:07.3
14:54:41.36 +47:58:02.0
14:52:42.49 +46:09:06.0
########### Completed Boo-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
15:38:04.43 +47:26:30.0
15:50:19.15 +46:30:00.7
15:57:30.36 +45:40:01.9
15:18:42.10 +47:33:03.4
16:04:38.42 +44:56:53.9
15:23:30.50 +47:40:32.7
14:56:50.29 +42:16:32.0
16:10:58.57 +42:51:21.0
15:20:10.25 +48:11:31.1
14:55:38.28 +45:28:54.1
15:31:13.64 +42:52:39.7
16:09:57.95 +41:28:40.1
15:38:19.33 +50:20:21.6
15:00:09.01 +48:49:44.1
15:59:55.00 +49:49:20.2
15:34:18.15 +49:29:52.0
16:06:45.80 +49:22:27.4
16:24:40.05 +49:45:56.9
15:59:52.90 +49:49:19.1
15:06:28.60 +46:20:39.7
16:25:00.18 +49:30:07.3
14:54:41.36 +47:58:02.0
14:52:42.49 +46:09:06.0
###################################################################################
15:38:04.43 +47:26:30.0 -- not an asteroid (will add it to exclusion list)
15:50:19.15 +46:30:00.7 -- not an asteroid (will add it to exclusion list)
15:57:30.36 +45:40:01.9 -- not an asteroid (will add it to exclusion list)
15:18:42.10 +47:33:03.4 -- not an asteroid (will add it to exclusion list)
16:04:38.42 +44:56:53.9 -- not an asteroid (will add it to exclusion list)
15:23:30.50 +47:40:32.7 -- not an asteroid (will add it to exclusion list)
14:56:50.29 +42:16:32.0 -- not an asteroid (will add it to exclusion list)
16:10:58.57 +42:51:21.0 -- not an asteroid (will add it to exclusion list)
15:20:10.25 +48:11:31.1 -- not an asteroid (will add it to exclusion list)
14:55:38.28 +45:28:54.1 -- not an asteroid (will add it to exclusion list)
15:31:13.64 +42:52:39.7 -- not an asteroid (will add it to exclusion list)
16:09:57.95 +41:28:40.1 -- not an asteroid (will add it to exclusion list)
15:38:19.33 +50:20:21.6 -- not an asteroid (will add it to exclusion list)
15:00:09.01 +48:49:44.1 -- not an asteroid (will add it to exclusion list)
15:59:55.00 +49:49:20.2 -- not an asteroid (will add it to exclusion list)
15:34:18.15 +49:29:52.0 -- not an asteroid (will add it to exclusion list)
16:06:45.80 +49:22:27.4 -- not an asteroid (will add it to exclusion list)
16:24:40.05 +49:45:56.9 -- not an asteroid (will add it to exclusion list)
15:59:52.90 +49:49:19.1 -- not an asteroid (will add it to exclusion list)
15:06:28.60 +46:20:39.7 -- not an asteroid (will add it to exclusion list)
16:25:00.18 +49:30:07.3 -- not an asteroid (will add it to exclusion list)
14:54:41.36 +47:58:02.0 -- not an asteroid (will add it to exclusion list)
14:52:42.49 +46:09:06.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
14:52:42.49 +46:09:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:54:41.36 +47:58:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:55:38.28 +45:28:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:56:50.29 +42:16:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:00:09.01 +48:49:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:06:28.60 +46:20:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:18:42.10 +47:33:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:20:10.25 +48:11:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:23:30.50 +47:40:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:13.64 +42:52:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:18.15 +49:29:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:38:04.43 +47:26:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:38:19.33 +50:20:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:19.15 +46:30:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:30.36 +45:40:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:52.90 +49:49:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:55.00 +49:49:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:04:38.42 +44:56:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:06:45.80 +49:22:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:09:57.95 +41:28:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:58.57 +42:51:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:40.05 +49:45:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:25:00.18 +49:30:07.3 -- 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)
14:52:42.49 +46:09:06.0 -- not a known variable star
14:54:41.36 +47:58:02.0 -- not a known variable star
14:55:38.28 +45:28:54.1 -- not a known variable star
14:56:50.29 +42:16:32.0 -- not a known variable star
15:00:09.01 +48:49:44.1 -- not a known variable star
15:06:28.60 +46:20:39.7 -- not a known variable star
15:18:42.10 +47:33:03.4 -- not a known variable star
15:20:10.25 +48:11:31.1 -- not a known variable star
15:23:30.50 +47:40:32.7 -- not a known variable star
15:31:13.64 +42:52:39.7 -- not a known variable star
15:34:18.15 +49:29:52.0 -- not a known variable star
15:38:04.43 +47:26:30.0 -- not a known variable star
15:38:19.33 +50:20:21.6 -- not a known variable star
15:50:19.15 +46:30:00.7 -- not a known variable star
15:57:30.36 +45:40:01.9 -- not a known variable star
15:59:52.90 +49:49:19.1 -- not a known variable star
15:59:55.00 +49:49:20.2 -- not a known variable star
16:04:38.42 +44:56:53.9 -- not a known variable star
16:06:45.80 +49:22:27.4 -- not a known variable star
16:09:57.95 +41:28:40.1 -- not a known variable star
16:10:58.57 +42:51:21.0 -- not a known variable star
16:24:40.05 +49:45:56.9 -- not a known variable star
16:25:00.18 +49:30:07.3 -- not a known variable star
Found 23 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
23 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
14:52:42.49 +46:09:06.0
14:54:41.36 +47:58:02.0
14:55:38.28 +45:28:54.1
14:56:50.29 +42:16:32.0
15:00:09.01 +48:49:44.1
15:06:28.60 +46:20:39.7
15:18:42.10 +47:33:03.4
15:20:10.25 +48:11:31.1
15:23:30.50 +47:40:32.7
15:31:13.64 +42:52:39.7
15:34:18.15 +49:29:52.0
15:38:04.43 +47:26:30.0
15:38:19.33 +50:20:21.6
15:50:19.15 +46:30:00.7
15:57:30.36 +45:40:01.9
15:59:52.90 +49:49:19.1
15:59:55.00 +49:49:20.2
16:04:38.42 +44:56:53.9
16:06:45.80 +49:22:27.4
16:09:57.95 +41:28:40.1
16:10:58.57 +42:51:21.0
16:24:40.05 +49:45:56.9
16:25:00.18 +49:30:07.3
16:25:34.40 +49:28:53.0
15:51:18.69 +43:58:07.0
15:35:00.21 +43:08:48.0
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461146.93209678 -observatory V36
00:09:35.16 -01:49:10.1 Mercury (0.0mag)
03:10:46.00 +18:01:07.5 Venus (-3.9mag)
00:19:04.40 +00:59:59.4 Mars (1.2mag)
07:12:49.65 +22:45:53.7 Jupiter (-2.1mag)
00:29:22.49 +00:50:10.8 Saturn (0.9mag)
03:47:47.30 +19:47:45.9 Uranus (5.8mag)
00:10:53.83 -00:15:01.0 Neptune (7.8mag)
20:33:46.43 -22:52:37.1 Pluto (14.5mag)
00:41:24.17 +06:40:36.6 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Apr 16 06:19 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461146.93209678:
07:12:57.32 +22:45:38.5 Io (5.8mag)
07:13:00.27 +22:45:32.6 Europa (5.9mag)
07:13:03.15 +22:45:20.1 Ganymede (5.4mag)
07:13:24.86 +22:44:40.5 Callisto (6.6mag)
07:16:08.77 +22:33:19.2 Himalia (15.3mag)
07:12:51.33 +22:45:52.1 Thebe (16.2mag)
07:16:20.71 +23:03:32.6 Elara (17.3mag)
07:11:44.34 +23:25:40.4 Pasiphae (17.4mag)
07:21:08.80 +22:43:57.5 Carme (18.5mag)
00:29:21.73 +00:50:37.9 Titan (8.8mag)
00:29:22.81 +00:50:11.9 Rhea (10.1mag)
00:29:01.77 +00:50:16.1 Iapetus (11.5mag)
00:29:29.26 +00:50:32.5 Hyperion (14.8mag)
00:30:59.04 +00:58:56.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 16 06:19 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461146.93209678:
15:39:12.33 -16:35:54.0 JWST
15:28:06.57 +53:12:09.1 Chandra
09:02:01.14 -51:24:35.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 16 06:19 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461146.93209678 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:10.59 -28:48:17.3 13.9mag P/2010 H2 (Vales)
05:07:02.85 -69:38:28.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:32.44 +31:26:24.8 17.2mag C/2017 K2 (PANSTARRS)
17:30:23.47 +10:35:55.8 17.6mag C/2021 G2 (ATLAS)
23:10:20.38 +29:14:46.3 17.1mag C/2022 E2 (ATLAS)
04:29:44.52 +26:02:59.8 16.0mag C/2022 N2 (PANSTARRS)
09:03:30.82 +32:01:11.3 16.2mag C/2022 QE78 (ATLAS)
08:31:08.42 -00:06:27.2 17.3mag C/2022 R6 (PANSTARRS)
18:53:37.64 +18:34:07.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:31.93 -11:30:55.1 17.5mag P/2023 B1 (PANSTARRS)
09:07:26.22 -11:48:50.8 17.6mag C/2023 F3 (ATLAS)
21:54:38.93 +62:55:55.7 17.5mag C/2023 H5 (Lemmon)
19:18:49.30 -03:44:23.3 14.1mag C/2023 R1 (PANSTARRS)
21:31:39.02 +85:58:18.8 17.8mag C/2023 X2 (Lemmon)
06:18:06.24 +63:30:38.5 17.2mag C/2024 A1 (ATLAS)
05:14:12.15 +18:27:01.2 11.1mag C/2024 E1 (Wierzchos)
16:18:59.75 +06:27:40.5 17.4mag C/2024 G6 (ATLAS)
20:20:55.89 +15:23:31.6 14.6mag C/2024 J3 (ATLAS)
03:26:45.52 -22:19:11.5 16.3mag C/2024 T5 (ATLAS)
05:17:04.92 +45:11:01.6 17.7mag C/2025 J1 (Borisov)
13:37:01.85 +45:46:02.1 15.2mag C/2025 L1 (ATLAS)
03:25:57.84 -26:16:45.2 17.8mag C/2025 Q3 (ATLAS)
23:47:22.84 +18:27:22.2 8.4mag C/2025 R3 (PANSTARRS)
12:53:55.76 +03:02:20.1 17.4mag C/2025 Y1 (ATLAS)
03:31:25.84 +02:34:29.6 13.4mag C/2026 A1 (MAPS)
00:00:48.43 +37:17:55.3 14.6mag C/2026 B2 (Sun-Gao)
18:43:46.45 -09:41:46.5 11.8mag 10P/Tempel
14:59:42.39 +03:09:50.4 14.0mag 24P/Schaumasse
11:02:41.21 -01:30:44.4 15.7mag 29P/Schwassmann-Wachmann
18:01:04.82 -09:35:40.5 18.0mag 40P/Vaisala
10:37:32.79 -04:03:53.2 16.9mag 43P/Wolf-Harrington
01:49:20.72 +17:33:40.2 17.2mag 47P/Ashbrook-Jackson
07:11:33.86 +36:55:08.5 17.0mag 63P/Wild
23:29:36.58 -11:23:56.9 15.7mag 65P/Gunn
04:04:24.60 +21:24:09.7 15.9mag 76P/West-Kohoutek-Ikemura
01:06:32.07 +08:18:48.8 14.3mag 78P/Gehrels
23:04:18.80 -09:15:48.4 14.6mag 88P/Howell
02:11:37.76 +20:45:25.7 15.1mag 93P/Lovas
04:55:37.36 +32:18:37.0 16.2mag 123P/West-Hartley
08:28:52.31 +38:09:38.7 16.2mag 124P/Mrkos
02:33:53.20 +14:25:05.0 16.4mag 128P/Shoemaker-Holt
02:48:23.30 +14:32:44.4 17.5mag 131P/Mueller
01:28:26.74 +13:23:12.2 10.6mag 141P/Machholz
01:37:18.80 +05:02:08.8 10.6mag 141P-A/Machholz
00:22:24.18 +00:55:47.6 12.8mag 141P-D/Machholz
02:07:40.57 +06:47:42.8 17.8mag 141P-I/Machholz
01:03:35.33 -01:18:29.7 15.1mag 162P/SidingSpring
14:50:39.51 -00:01:26.2 17.7mag 210P/Christensen
21:40:05.72 -11:20:41.6 17.6mag 218P/LINEAR
17:16:39.95 -13:52:53.6 16.1mag 235P/LINEAR
05:35:25.15 +34:43:50.6 16.8mag 240P/NEAT
07:38:42.48 -05:07:14.0 17.7mag 242P/Spahr
22:17:59.54 -20:51:53.7 17.9mag 260P/McNaught
01:59:04.51 +20:34:08.8 18.0mag 295P/LINEAR
15:42:28.42 +07:01:08.0 17.5mag 391P/Kowalski
07:34:21.81 +21:22:01.6 17.7mag 450P/LONEOS
05:36:30.24 +45:00:25.3 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 16 06:19 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
15:25:54.99 +07:49:24.50 2026-04-12.14 16.96
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
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
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
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
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
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
-rw-r--r-- 1 apache apache 5.8K Apr 16 06:19 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 16 06:19 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:32:40.720 +02:42:54.71 AT 2026jay 2026-04-06.66 22
14:07:18.110 +04:13:29.83 AT 2026jax 2026-04-06.66 22.26
14:14:08.750 +03:35:26.74 AT 2026jaw 2026-04-06.66 22.24
14:03:53.740 +04:33:03.03 AT 2026jav 2026-04-06.66 22.18
14:07:43.620 +03:35:48.12 AT 2026jau 2026-04-06.66 21.82
14:10:23.930 -01:02:22.49 AT 2026jat 2026-04-06.65 22.15
13:51:42.460 +03:14:48.63 AT 2026jas 2026-04-06.65 21.87
13:42:53.750 +01:22:24.17 AT 2026jar 2026-04-06.65 22.6
13:44:21.040 -01:54:42.32 AT 2026jaq 2026-04-06.65 22.71
13:35:29.290 +00:58:49.10 AT 2026jap 2026-04-06.64 22.39
13:41:45.110 +04:07:23.04 AT 2026jao 2026-04-06.64 21.84
13:38:11.980 +03:37:12.11 AT 2026jan 2026-04-06.64 22.48
13:27:27.970 +05:34:49.94 AT 2026jam 2026-04-06.64 21.79
13:28:44.170 +03:09:01.26 AT 2026jal 2026-04-06.64 22.01
13:29:02.030 -02:11:15.98 AT 2026jak 2026-04-06.64 21.54
13:11:37.460 +01:53:43.84 AT 2026jaj 2026-04-06.63 21.95
13:13:23.110 +00:38:42.68 AT 2026jai 2026-04-06.63 21.88
13:19:01.640 +03:04:08.10 AT 2026jah 2026-04-06.63 22.02
13:06:29.860 +02:34:35.75 AT 2026jag 2026-04-06.63 22.28
13:04:16.080 -00:23:58.35 AT 2026jaf 2026-04-06.63 22.55
-rw-r--r-- 1 apache apache 30K Apr 16 06:19 tns_transients_list.txt
