This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL
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 477969391203931136,2461144.7092,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477969391203931136 20260414.2092 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 479417791611935360,2461144.7092,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 479417791611935360 20260414.2092 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461144.7092,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2092 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.7092,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2092 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.7092,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2092 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.7092,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2092 13.03CV 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 478182833898536576,2461144.7092,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478182833898536576 20260414.2092 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 285656694309094016,2461144.7092,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 285656694309094016 20260414.2092 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 477829443988647680,2461144.7092,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477829443988647680 20260414.2092 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 285837529613169920,2461144.7092,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 285837529613169920 20260414.2092 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 478284740584103168,2461144.7092,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478284740584103168 20260414.2092 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 477978286077526400,2461144.7092,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477978286077526400 20260414.2092 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 477986055676141824,2461144.7092,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477986055676141824 20260414.2092 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 287394511094533376,2461144.7092,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287394511094533376 20260414.2092 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 478232376343406464,2461144.7092,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478232376343406464 20260414.2092 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 14.2092 2461144.7092 12.48 05:19:29.26 +59:14:39.8
151.74446 12.36356 galactic Cam Second-epoch detections are separated by 4.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 281344963758263936 | 05:19:29.39 +59:14:30.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F7 (LAMOST DR5)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
Large-amplitude variable Gaia DR2 281344963758263936,2461144.7092,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 281344963758263936 20260414.2092 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 478356144419398912,2461144.7092,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478356144419398912 20260414.2092 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 478068858347848448,2461144.7092,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478068858347848448 20260414.2092 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050148.09+623831.2,2461144.7092,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050148.09+623831.2 20260414.2092 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 477972685440184448,2461144.7092,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477972685440184448 20260414.2092 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 283479012749540352,2461144.7092,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 283479012749540352 20260414.2092 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 477912766353894912,2461144.7092,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477912766353894912 20260414.2092 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!
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 477961866420396928,2461144.7092,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477961866420396928 20260414.2092 12.29CV 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 477656610206912384,2461144.7092,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477656610206912384 20260414.2092 12.29CV 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 477969940959046528,2461144.7092,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477969940959046528 20260414.2092 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 478226638266436224,2461144.7092,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478226638266436224 20260414.2092 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 478247670724819328,2461144.7092,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478247670724819328 20260414.2092 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 280258714990705408,2461144.7092,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 280258714990705408 20260414.2092 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 478045772901464832,2461144.7092,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 478045772901464832 20260414.2092 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 286851730307777408,2461144.7092,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286851730307777408 20260414.2092 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
KK Cam,2461144.7092,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KK Cam 20260414.2092 11.30CV 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,2461144.7092,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2092 13.38CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461144.70955420 14.04.2026 05:01:35.483 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 14295
Objects passed selection criteria: 14213
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 9099.25
Average stars matched: 8558 (94.0517 %)
Memory usage VmPeak: 119540 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 00:05:36 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: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461144.70955420 14.04.2026 05:01:35.483 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 109
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 28 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 101899
Objects passed selection criteria: 101519
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 64060.8
Average stars matched: 60076 (93.7797 %)
Memory usage VmPeak: 1937192 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 00:07:54 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461144.70893108
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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
Saving wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits to local_wcs_cache/
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
Saving wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits to local_wcs_cache/
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits'
wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:45.003 +62:04:10.54
Angular distance between the image centers 0.0795 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:45.288 +62:03:43.57
Angular distance between the image centers 0.0730 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 05:08:45.003 +62:04:10.54
Second-epoch second image center 05:08:45.288 +62:03:43.57
Angular distance between the image centers 0.00751 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/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.FcqvoukpHt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.nGu0pTkec2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits &> /tmp/tmp.t2ixMeogGt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits &> /tmp/tmp.Rb5qDCetH5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
The reference image (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat) found
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat' -> 'wcsmag.cat'
Read 18409 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 57.0231 to 95.6672 deg, Dec +55.2649 to +67.4913 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 57.0231 to 95.6672 deg, Dec 55.2649 to 67.4913 deg
Loaded 14048 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): 8129 out of 8891 total matches.
Matched with Tycho-2 8891 out of 18409 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955063
a=0.000000 b=1.000000 c=22.955063
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
2.0 pix Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
4.7 pix fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
4.7 pix fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Limiting magnitude estimates:
15.5 mag. Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.5 mag. Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
13.6 mag. fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
13.6 mag. fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FcqvoukpHt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1604, passed=18409
Got 18409 stars (including 16782 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 18409 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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18199 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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.nGu0pTkec2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1596, passed=18487
Got 18487 stars (including 16865 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 18487 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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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.t2ixMeogGt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=412, passed=6170
Got 6170 stars (including 5756 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat
util/solve_plate_with_UCAC5 got 6170 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 6091 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.04"
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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 6092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.03"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 6092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Excluding outliers - 948 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.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.Rb5qDCetH5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=387, passed=6117
Got 6117 stars (including 5728 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat
util/solve_plate_with_UCAC5 got 6117 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.04"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 6036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.05"
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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 6037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.03"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 6037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
Saving fully-calibrated image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits'
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits'
Preparing the HTML report for the field Cam-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21709.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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: 2s
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Considering the candidate 20884_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 20884_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21709_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 21709_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 08746_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 08746_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:13:02.65 +61:51:00.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07693_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 07693_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:01:36.17 +61:04:38.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07622_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 07622_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:06:29.63 +61:10:11.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04490_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 04490_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:15:11.38 +59:24:22.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09859_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 09859_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:20:21.95 +62:39:13.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06470_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 06470_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:03:24.97 +60:26:36.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04064_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 04064_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:06:12.10 +59:01:20.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12435_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 12435_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:37:15.01 +64:09:14.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07782_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 07782_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:44:08.31 +61:28:35.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12026_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 12026_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:52:05.80 +63:30:15.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10489_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 10489_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:30:09.16 +63:03:59.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03981_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 03981_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:06:08.38 +58:58:26.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15068_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 15068_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:42:25.58 +65:41:47.3 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 17s
Prepared the HTML report for the field Cam-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:04:23.54 +62:24:19.2
05:06:17.58 +65:11:56.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Creating symlink local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits exists and is non-empty
wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:45.003 +62:04:10.54
Angular distance between the image centers 0.0795 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:45.288 +62:03:43.57
Angular distance between the image centers 0.0730 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 05:08:45.003 +62:04:10.54
Second-epoch second image center 05:08:45.288 +62:03:43.57
Angular distance between the image centers 0.00751 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/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.TCKc3sdiHX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.JuyrpuICnt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits &> /tmp/tmp.3VH0UIR7p4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits &> /tmp/tmp.08x0bT9Ul8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
The reference image (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat) found
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat' -> 'wcsmag.cat'
Read 131449 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 56.9471 to 95.6842 deg, Dec +55.1951 to +67.5012 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 56.9471 to 95.6842 deg, Dec 55.1951 to 67.5012 deg
Loaded 14165 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): 6817 out of 9000 total matches.
Matched with Tycho-2 9000 out of 131449 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.808691
a=0.000000 b=1.000000 c=22.808691
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 82 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
1.9 pix Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
3.7 pix fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
3.7 pix fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Limiting magnitude estimates:
15.6 mag. Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.6 mag. Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
13.9 mag. fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
13.9 mag. fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.1 (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.TCKc3sdiHX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=12667, passed=131418
Got 131418 stars (including 118531 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 131418 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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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.JuyrpuICnt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=12449, passed=130538
Got 130538 stars (including 117858 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 130538 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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129188 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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.3VH0UIR7p4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=4122, passed=32480
Got 32480 stars (including 28319 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat
util/solve_plate_with_UCAC5 got 32480 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 32121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.06"
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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 32121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.06"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 32120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 951 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.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.08x0bT9Ul8 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=4083, passed=32508
Got 32508 stars (including 28380 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat
util/solve_plate_with_UCAC5 got 32508 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 32185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.08"
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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 32186 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.07"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 32186 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Saving fully-calibrated image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-00-41_20.00sec_-4.90C_LIGHT_0779.fits
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-09-Q2b1x1_000227_TTUQ2b1x1_15521_Pbo0snhL/wcs_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780.fits
Preparing the HTML report for the field Cam-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out150677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out121037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93507.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 43s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 17s
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Considering the candidate 150655_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150655_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 150660_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150660_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150662_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150662_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150675_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150675_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150677_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150677_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:46:18.23 +62:04:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 5.639 477764469723126784 071.57319414304 +62.06796473371 12.4011 11.3843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150686_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150686_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150716_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150716_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:01:08.80 +62:10:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.325 477590227192401280 075.28490838731 +62.17498844278 12.4041 11.8151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150718_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150718_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:20:21.01 +62:17:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.501 285672602869630336 080.08756195165 +62.28808311249 12.3601 11.6424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150732_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150732_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:36:51.64 +64:10:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.187 476161587930942336 069.21581453564 +64.17832941485 13.0072 12.4080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150735_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150735_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:10:56.16 +62:48:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.388 477996118783630464 077.73345647703 +62.81342728427 12.5032 11.9505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150736_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150736_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 150738_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150738_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:57:46.56 +61:57:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.725 477604933161382400 074.44380984640 +61.95141834533 12.1698 11.2144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150740_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150740_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:05:36.73 +62:41:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150744_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150744_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:03:06.15 +61:43:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.637 285409647790860288 075.77407480227 +61.72908376034 12.4575 11.8769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150755_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150755_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:02:36.00 +61:32:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150758_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150758_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150768_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150768_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150777_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150777_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150778_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150778_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150781_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150781_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:11:49.63 +61:41:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 5.695 285548564214065152 077.95348372295 +61.68628532972 12.2998 11.7033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150782_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150782_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:58:57.30 +63:43:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.374 478717226610852608 074.73842710718 +63.73137314192 12.1764 11.2583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150783_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150783_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:00:32.10 +61:55:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.414 477566106657030912 075.13493920607 +61.91646472339 11.8268 11.1342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150786_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150786_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:03:31.92 +61:53:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.045 285789563418022912 075.88441155325 +61.89407808724 12.2361 11.7051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150800_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150800_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:01:19.45 +61:57:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 5.398 477571947812549632 075.33149313255 +61.95054349119 12.1582 11.6145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150806_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150806_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150807_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150807_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150817_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150817_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150818_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150818_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150822_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150822_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150825_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150825_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150826_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150826_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150831_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150831_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150832_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150832_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150833_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150833_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:36:12.80 +64:59:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.877 482260853807692544 069.05279874530 +64.99422442490 12.2299 11.3123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150834_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150834_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150839_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150839_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 150840_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150840_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150841_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150841_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 150854_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150854_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150855_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 150855_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:16:00.64 +62:11:42.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 150857_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150857_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150864_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150864_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150867_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150867_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150868_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150868_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150869_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150869_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150870_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150870_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 150877_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 150877_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 154382_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 154382_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 81783_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 81783_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 56549_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 56549_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 121037_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 121037_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 93507_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
Preparing report for the candidate 93507_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
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Considering the candidate 81178_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 81178_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:14:38.54 +63:07:37.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 73742_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 73742_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:09:40.11 +62:28:45.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 42088_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 42088_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:17:27.46 +60:10:51.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 65419_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 65419_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:57:15.38 +61:45:11.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 125422_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 125422_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:50:10.04 +63:37:30.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 76053_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 76053_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:13:31.12 +62:41:28.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129659_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 129659_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:10:42.86 +63:35:48.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 64558_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 64558_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:13:02.63 +61:51:01.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 63932_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 63932_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:53:39.82 +61:28:53.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 55788_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 55788_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:06:29.62 +61:10:11.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 41721_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 41721_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:29:51.70 +60:16:06.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 56673_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 56673_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:01:36.18 +61:04:38.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 72637_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 72637_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:20:21.99 +62:39:13.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 46344_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 46344_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:03:24.98 +60:26:36.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 108949_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 108949_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:46:24.76 +64:48:34.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 112947_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 112947_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:09:44.30 +64:55:04.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106069_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 106069_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:57:31.74 +65:16:39.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 126795_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 126795_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:52:05.80 +63:30:15.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32056_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 32056_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:15:11.36 +59:24:22.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 78190_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 78190_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:30:09.16 +63:03:59.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 28801_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 28801_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:06:12.12 +59:01:20.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 28091_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 28091_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:06:08.38 +58:58:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31948_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 31948_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:57:09.64 +59:07:16.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 61294_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 61294_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:38:15.37 +60:53:04.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 125334_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 125334_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:37:14.99 +64:09:15.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 57388_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 57388_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:44:08.33 +61:28:36.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14999_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 14999_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:19:27.80 +58:07:04.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112882_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 112882_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 04:36:24.50 +64:15:40.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117216_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 117216_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:46:12.35 +64:46:08.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104727_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780
The candidate 104727_fd_Cam-09-Q2b1x1_2026-04-14_00-01-35_20.00sec_-4.90C_LIGHT_0780 did not pass the final checks
**** FOUND 05:42:25.54 +65:41:47.1 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 62s
Prepared the HTML report for the field Cam-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:04:23.54 +62:24:19.2
05:06:17.58 +65:11:56.6
05:19:47.19 +64:26:00.3
05:32:35.27 +61:49:31.5
04:52:11.99 +64:23:55.5
05:18:22.80 +59:30:46.3
05:23:22.27 +62:12:47.3
05:13:00.91 +63:30:59.2
05:15:56.42 +62:07:35.6
04:54:03.70 +62:25:40.2
05:11:19.11 +62:39:33.1
05:05:21.92 +63:28:01.3
05:06:36.15 +62:36:59.6
05:07:33.93 +62:33:21.5
05:22:45.67 +63:01:03.2
05:01:51.74 +62:56:12.2
05:19:29.26 +59:14:39.8
05:05:46.76 +63:52:26.5
05:06:07.85 +62:57:45.7
05:01:47.05 +62:38:24.5
05:05:31.45 +62:27:26.3
05:45:42.45 +61:50:52.2
04:57:58.24 +62:51:52.7
05:06:36.07 +62:27:33.7
05:01:23.01 +62:27:39.1
05:03:49.18 +62:24:06.9
05:02:14.14 +62:46:07.3
05:03:06.47 +63:07:56.4
05:24:58.06 +58:13:12.4
05:04:04.91 +62:49:36.1
05:44:14.47 +63:12:29.6
04:53:34.00 +62:48:07.4
########### Completed Cam-09-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:04:23.54 +62:24:19.2
05:06:17.58 +65:11:56.6
05:32:35.27 +61:49:31.5
04:52:11.99 +64:23:55.5
05:18:22.80 +59:30:46.3
05:23:22.27 +62:12:47.3
05:13:00.91 +63:30:59.2
05:15:56.42 +62:07:35.6
04:54:03.70 +62:25:40.2
05:11:19.11 +62:39:33.1
05:05:21.92 +63:28:01.3
05:06:36.15 +62:36:59.6
05:07:33.93 +62:33:21.5
05:22:45.67 +63:01:03.2
05:01:51.74 +62:56:12.2
05:19:29.26 +59:14:39.8
05:05:46.76 +63:52:26.5
05:06:07.85 +62:57:45.7
05:01:47.05 +62:38:24.5
05:05:31.45 +62:27:26.3
05:45:42.45 +61:50:52.2
04:57:58.24 +62:51:52.7
05:06:36.07 +62:27:33.7
05:01:23.01 +62:27:39.1
05:03:49.18 +62:24:06.9
05:02:14.14 +62:46:07.3
05:03:06.47 +63:07:56.4
05:24:58.06 +58:13:12.4
05:04:04.91 +62:49:36.1
05:44:14.47 +63:12:29.6
05:19:47.19 +64:26:00.3
04:53:34.00 +62:48:07.4
###################################################################################
05:04:23.54 +62:24:19.2 -- not an asteroid (will add it to exclusion list)
05:06:17.58 +65:11:56.6 -- not an asteroid (will add it to exclusion list)
05:32:35.27 +61:49:31.5 -- not an asteroid (will add it to exclusion list)
04:52:11.99 +64:23:55.5 -- not an asteroid (will add it to exclusion list)
05:18:22.80 +59:30:46.3 -- not an asteroid (will add it to exclusion list)
05:23:22.27 +62:12:47.3 -- not an asteroid (will add it to exclusion list)
05:13:00.91 +63:30:59.2 -- not an asteroid (will add it to exclusion list)
05:15:56.42 +62:07:35.6 -- not an asteroid (will add it to exclusion list)
04:54:03.70 +62:25:40.2 -- not an asteroid (will add it to exclusion list)
05:11:19.11 +62:39:33.1 -- not an asteroid (will add it to exclusion list)
05:05:21.92 +63:28:01.3 -- not an asteroid (will add it to exclusion list)
05:06:36.15 +62:36:59.6 -- not an asteroid (will add it to exclusion list)
05:07:33.93 +62:33:21.5 -- not an asteroid (will add it to exclusion list)
05:22:45.67 +63:01:03.2 -- not an asteroid (will add it to exclusion list)
05:01:51.74 +62:56:12.2 -- not an asteroid (will add it to exclusion list)
05:19:29.26 +59:14:39.8 -- not an asteroid (will add it to exclusion list)
05:05:46.76 +63:52:26.5 -- not an asteroid (will add it to exclusion list)
05:06:07.85 +62:57:45.7 -- not an asteroid (will add it to exclusion list)
05:01:47.05 +62:38:24.5 -- not an asteroid (will add it to exclusion list)
05:05:31.45 +62:27:26.3 -- not an asteroid (will add it to exclusion list)
05:45:42.45 +61:50:52.2 -- not an asteroid (will add it to exclusion list)
04:57:58.24 +62:51:52.7 -- not an asteroid (will add it to exclusion list)
05:06:36.07 +62:27:33.7 -- not an asteroid (will add it to exclusion list)
05:01:23.01 +62:27:39.1 -- not an asteroid (will add it to exclusion list)
05:03:49.18 +62:24:06.9 -- not an asteroid (will add it to exclusion list)
05:02:14.14 +62:46:07.3 -- not an asteroid (will add it to exclusion list)
05:03:06.47 +63:07:56.4 -- not an asteroid (will add it to exclusion list)
05:24:58.06 +58:13:12.4 -- not an asteroid (will add it to exclusion list)
05:04:04.91 +62:49:36.1 -- not an asteroid (will add it to exclusion list)
05:44:14.47 +63:12:29.6 -- not an asteroid (will add it to exclusion list)
05:19:47.19 +64:26:00.3 -- not an asteroid (will add it to exclusion list)
04:53:34.00 +62:48:07.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:52:11.99 +64:23:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:34.00 +62:48:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:03.70 +62:25:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:58.24 +62:51:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:23.01 +62:27:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:47.05 +62:38:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:51.74 +62:56:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:14.14 +62:46:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:06.47 +63:07:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:49.18 +62:24:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:04.91 +62:49:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:23.54 +62:24:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:21.92 +63:28:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:31.45 +62:27:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:46.76 +63:52:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:07.85 +62:57:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:17.58 +65:11:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:36.07 +62:27:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:36.15 +62:36:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:33.93 +62:33:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:19.11 +62:39:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:00.91 +63:30:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:56.42 +62:07:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:22.80 +59:30:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:29.26 +59:14:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:47.19 +64:26:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:45.67 +63:01:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:22.27 +62:12:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:58.06 +58:13:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:35.27 +61:49:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:14.47 +63:12:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:42.45 +61:50:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
04:52:11.99 +64:23:55.5 -- not a known variable star
04:53:34.00 +62:48:07.4 -- not a known variable star
04:54:03.70 +62:25:40.2 -- not a known variable star
04:57:58.24 +62:51:52.7 -- not a known variable star
05:01:23.01 +62:27:39.1 -- not a known variable star
05:01:47.05 +62:38:24.5 -- a known variable star
05:01:51.74 +62:56:12.2 -- not a known variable star
05:02:14.14 +62:46:07.3 -- not a known variable star
05:03:06.47 +63:07:56.4 -- not a known variable star
05:03:49.18 +62:24:06.9 -- not a known variable star
05:04:04.91 +62:49:36.1 -- not a known variable star
05:04:23.54 +62:24:19.2 -- not a known variable star
05:05:21.92 +63:28:01.3 -- not a known variable star
05:05:31.45 +62:27:26.3 -- not a known variable star
05:05:46.76 +63:52:26.5 -- not a known variable star
05:06:07.85 +62:57:45.7 -- not a known variable star
05:06:17.58 +65:11:56.6 -- not a known variable star
05:06:36.07 +62:27:33.7 -- not a known variable star
05:06:36.15 +62:36:59.6 -- not a known variable star
05:07:33.93 +62:33:21.5 -- not a known variable star
05:11:19.11 +62:39:33.1 -- not a known variable star
05:13:00.91 +63:30:59.2 -- not a known variable star
05:15:56.42 +62:07:35.6 -- not a known variable star
05:18:22.80 +59:30:46.3 -- not a known variable star
05:19:29.26 +59:14:39.8 -- not a known variable star
05:19:47.19 +64:26:00.3 -- a known variable star
05:22:45.67 +63:01:03.2 -- not a known variable star
05:23:22.27 +62:12:47.3 -- not a known variable star
05:24:58.06 +58:13:12.4 -- not a known variable star
05:32:35.27 +61:49:31.5 -- not a known variable star
05:44:14.47 +63:12:29.6 -- not a known variable star
05:45:42.45 +61:50:52.2 -- not a known variable star
Found 30 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
32 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
04:52:11.99 +64:23:55.5
04:53:34.00 +62:48:07.4
04:54:03.70 +62:25:40.2
04:57:58.24 +62:51:52.7
05:01:23.01 +62:27:39.1
05:01:47.05 +62:38:24.5
05:01:51.74 +62:56:12.2
05:02:14.14 +62:46:07.3
05:03:06.47 +63:07:56.4
05:03:49.18 +62:24:06.9
05:04:04.91 +62:49:36.1
05:04:23.54 +62:24:19.2
05:05:21.92 +63:28:01.3
05:05:31.45 +62:27:26.3
05:05:46.76 +63:52:26.5
05:06:07.85 +62:57:45.7
05:06:17.58 +65:11:56.6
05:06:36.07 +62:27:33.7
05:06:36.15 +62:36:59.6
05:07:33.93 +62:33:21.5
05:11:19.11 +62:39:33.1
05:13:00.91 +63:30:59.2
05:15:56.42 +62:07:35.6
05:18:22.80 +59:30:46.3
05:19:29.26 +59:14:39.8
05:19:47.19 +64:26:00.3
05:22:45.67 +63:01:03.2
05:23:22.27 +62:12:47.3
05:24:58.06 +58:13:12.4
05:32:35.27 +61:49:31.5
05:44:14.47 +63:12:29.6
05:45:42.45 +61:50:52.2
04:46:18.23 +62:04:01.5
05:01:08.80 +62:10:26.8
05:20:21.01 +62:17:18.6
04:36:51.64 +64:10:42.6
05:10:56.16 +62:48:49.4
04:57:46.56 +61:57:02.4
05:03:06.15 +61:43:47.2
05:11:49.63 +61:41:09.9
04:58:57.30 +63:43:48.6
05:00:32.10 +61:55:03.2
05:03:31.92 +61:53:36.8
05:01:19.45 +61:57:07.3
04:36:12.80 +64:59:40.9
05:16:00.64 +62:11:42.6
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461144.70893108 -observatory V36
23:57:58.22 -03:00:55.3 Mercury (0.1mag)
02:59:54.66 +17:10:29.1 Venus (-3.9mag)
00:12:45.19 +00:18:16.8 Mars (1.2mag)
07:11:49.97 +22:47:31.9 Jupiter (-2.1mag)
00:28:22.90 +00:43:59.4 Saturn (0.9mag)
03:47:19.34 +19:46:16.4 Uranus (5.8mag)
00:10:36.31 -00:16:51.2 Neptune (7.8mag)
20:33:40.41 -22:52:31.5 Pluto (14.5mag)
22:49:00.87 -07:42:25.1 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Apr 14 00:05 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461144.70893108:
07:11:47.46 +22:47:39.3 Io (5.8mag)
07:11:47.84 +22:47:33.3 Europa (5.9mag)
07:11:59.09 +22:47:19.5 Ganymede (5.3mag)
07:12:16.64 +22:46:44.3 Callisto (6.6mag)
07:15:14.86 +22:35:59.9 Himalia (15.3mag)
07:11:46.06 +22:47:40.3 Thebe (16.2mag)
07:15:23.91 +23:06:02.8 Elara (17.3mag)
07:10:35.55 +23:28:28.4 Pasiphae (17.4mag)
07:20:12.05 +22:45:22.4 Carme (18.5mag)
00:28:30.78 +00:44:15.8 Titan (8.8mag)
00:28:24.77 +00:44:13.5 Rhea (10.1mag)
00:28:06.14 +00:44:26.0 Iapetus (11.5mag)
00:28:36.13 +00:44:08.5 Hyperion (14.8mag)
00:30:01.21 +00:52:59.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 14 00:05 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.70893108:
15:30:13.45 -14:58:52.8 JWST
17:08:44.02 +44:07:50.7 Chandra
08:04:42.67 -40:04:32.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 14 00:05 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.70893108 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:15.07 -28:40:29.0 13.9mag P/2010 H2 (Vales)
05:05:27.46 -69:44:49.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:03.86 +31:25:31.1 17.2mag C/2017 K2 (PANSTARRS)
17:30:36.10 +10:20:06.6 17.6mag C/2021 G2 (ATLAS)
23:09:44.54 +29:09:30.3 17.1mag C/2022 E2 (ATLAS)
04:27:09.15 +25:59:22.7 16.0mag C/2022 N2 (PANSTARRS)
09:03:02.85 +32:00:21.6 16.2mag C/2022 QE78 (ATLAS)
08:30:48.40 -00:20:36.9 17.3mag C/2022 R6 (PANSTARRS)
18:54:08.81 +18:22:54.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:14.87 -11:32:52.0 17.5mag P/2023 B1 (PANSTARRS)
09:08:28.70 -12:10:15.8 17.6mag C/2023 F3 (ATLAS)
21:52:23.95 +62:48:08.0 17.5mag C/2023 H5 (Lemmon)
19:20:43.16 -03:42:14.1 14.2mag C/2023 R1 (PANSTARRS)
21:35:50.23 +85:39:50.5 17.8mag C/2023 X2 (Lemmon)
06:17:05.21 +63:31:17.2 17.1mag C/2024 A1 (ATLAS)
05:09:24.48 +17:42:05.7 10.9mag C/2024 E1 (Wierzchos)
16:20:25.12 +06:05:48.5 17.4mag C/2024 G6 (ATLAS)
20:20:18.00 +14:47:21.7 14.6mag C/2024 J3 (ATLAS)
03:24:45.82 -22:39:32.3 16.4mag C/2024 T5 (ATLAS)
05:15:11.86 +45:44:15.8 17.7mag C/2025 J1 (Borisov)
13:46:16.75 +44:16:53.9 15.1mag C/2025 L1 (ATLAS)
03:22:27.34 -25:56:00.5 17.8mag C/2025 Q3 (ATLAS)
23:29:01.92 +19:08:01.3 8.8mag C/2025 R3 (PANSTARRS)
12:54:53.71 +02:54:12.4 17.4mag C/2025 Y1 (ATLAS)
03:12:31.22 +02:49:47.2 12.7mag C/2026 A1 (MAPS)
23:54:28.88 +36:53:10.6 14.5mag C/2026 B2 (Sun-Gao)
18:39:26.97 -09:48:53.2 11.9mag 10P/Tempel
15:02:43.47 +03:23:36.1 13.8mag 24P/Schaumasse
11:03:17.25 -01:35:03.3 15.7mag 29P/Schwassmann-Wachmann
18:00:25.11 -09:40:35.4 17.9mag 40P/Vaisala
10:37:39.34 -04:14:33.3 16.9mag 43P/Wolf-Harrington
01:45:54.08 +17:10:55.3 17.2mag 47P/Ashbrook-Jackson
07:07:28.07 +37:23:49.3 17.0mag 63P/Wild
23:26:46.14 -11:39:59.1 15.7mag 65P/Gunn
03:58:28.39 +20:38:12.2 15.9mag 76P/West-Kohoutek-Ikemura
01:01:37.03 +07:52:35.2 14.3mag 78P/Gehrels
22:57:33.98 -09:55:14.7 14.6mag 88P/Howell
02:05:20.36 +20:09:48.3 15.1mag 93P/Lovas
04:51:26.17 +32:11:29.9 16.2mag 123P/West-Hartley
08:26:16.28 +39:11:15.5 16.2mag 124P/Mrkos
02:30:26.95 +14:10:11.7 16.4mag 128P/Shoemaker-Holt
02:44:01.44 +14:16:26.5 17.5mag 131P/Mueller
01:16:46.43 +12:36:52.1 10.7mag 141P/Machholz
01:25:56.91 +04:12:04.9 10.7mag 141P-A/Machholz
00:12:06.88 +00:10:40.6 13.0mag 141P-D/Machholz
01:56:07.29 +05:57:16.0 17.8mag 141P-I/Machholz
00:57:23.03 -02:25:35.4 15.1mag 162P/SidingSpring
10:29:05.67 +30:57:16.3 18.0mag 164P/Christensen
06:33:13.13 +24:17:53.3 18.0mag 198P/ODAS
14:54:37.12 -00:15:18.3 17.6mag 210P/Christensen
21:33:38.27 -11:52:50.1 17.6mag 218P/LINEAR
17:16:05.40 -14:08:53.1 16.1mag 235P/LINEAR
05:30:37.04 +34:33:41.0 16.7mag 240P/NEAT
07:37:37.28 -05:21:43.4 17.7mag 242P/Spahr
22:12:25.95 -21:27:13.7 17.9mag 260P/McNaught
15:43:20.06 +06:52:18.5 17.5mag 391P/Kowalski
07:33:30.95 +21:21:36.4 17.7mag 450P/LONEOS
05:33:15.74 +45:08:15.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 14 00:05 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
-rw-r--r-- 1 apache apache 5.8K Apr 14 00:05 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
-rw-r--r-- 1 apache apache 188K Apr 14 00:05 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:56:46.937 +30:48:49.43 AT 2026ivi 2026-04-07.29 20.1063
12:16:21.919 +30:21:04.60 AT 2026ivh 2026-04-07.29 19.651
09:11:45.682 +30:03:32.51 AT 2026ivg 2026-04-04.17 19.5142
09:55:25.809 -27:42:27.02 AT 2026ivf 2026-04-08.21 18.51
09:46:07.094 +07:14:13.61 AT 2026ive 2026-04-08.15 19.9446
09:29:29.340 -01:21:08.51 AT 2026ivd 2026-04-05.15 19.4593
09:53:27.521 +16:01:50.20 AT 2026ivc 2026-04-07.17 20.1328
10:57:27.283 +18:19:29.99 AT 2026ivb 2026-04-07.87 19.71
12:50:08.105 +01:17:40.78 AT 2026iva 2026-04-07.89 19.96
10:38:31.370 -04:47:42.62 AT 2026iuz 2026-04-07.85 18.9
13:03:44.252 +20:35:06.20 AT 2026iuy 2026-04-06.96 19.7
13:53:33.216 -46:24:12.81 AT 2026iux 2026-04-07.63 19.83
20:29:30.119 -10:56:33.33 AT 2026iuw 2026-03-29.79 19.55
13:31:30.960 -32:00:09.92 AT 2026iuv 2026-04-07.60 18.91
14:00:56.468 -25:06:29.29 AT 2026iuu 2026-04-07.35 18.482
13:27:25.132 +09:30:53.72 AT 2026iut 2026-04-05.33 19.4971
13:57:28.106 -31:36:18.49 AT 2026ius 2026-04-07.61 19.27
09:54:32.050 -01:17:25.84 SN 2026iur 2026-04-07.01 15.9
14:24:08.131 +22:56:14.71 AT 2026iuq 2026-04-07.38 19.91
10:07:28.221 -17:12:04.00 AT 2026iup 2026-04-05.31 20.26
-rw-r--r-- 1 apache apache 30K Apr 14 00:05 tns_transients_list.txt
