This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ
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
target,2461146.9603,14.43,0.05,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 20260416.4603 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.4603 14.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2121845,2461146.9603,14.40,0.05,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
DocumentRef: VOTx2121845 20260416.4603 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2213812,2461146.9603,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2213812 20260416.4603 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1796279194341463680,2461146.9603,14.29,0.05,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 1796279194341463680 20260416.4603 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.4603 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.14,0.05,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 20260416.4603 14.14CV 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 1799377927347451648,2461146.9603,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1799377927347451648 20260416.4603 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.6393+25.0132,2461146.9603,13.11,0.05,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
ATO J327.6393+25.0132 20260416.4603 13.11CV 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
DocumentRef: VOTx2125059,2461146.9603,13.62,0.05,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
DocumentRef: VOTx2125059 20260416.4603 13.62CV 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
target,2461146.9603,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.4603 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2653358,2461146.9603,14.02,0.05,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
DocumentRef: VOTx2653358 20260416.4603 14.02CV 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
DocumentRef: VOTx2487678,2461146.9603,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2487678 20260416.4603 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2584649,2461146.9603,14.22,0.05,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
DocumentRef: VOTx2584649 20260416.4603 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.4603 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CSS_J220346.6+202530,2461146.9603,14.22,0.05,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
CSS_J220346.6+202530 20260416.4603 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.28,0.05,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 20260416.4603 14.28CV 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
DocumentRef: VOTx3061074,2461146.9603,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3061074 20260416.4603 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3123393,2461146.9603,14.29,0.05,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
DocumentRef: VOTx3123393 20260416.4603 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.16,0.05,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 20260416.4603 14.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.23,0.05,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 20260416.4603 14.23CV 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
DocumentRef: VOTx3166292,2461146.9603,14.39,0.05,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
DocumentRef: VOTx3166292 20260416.4603 14.39CV 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 1780708185545540736,2461146.9603,14.29,0.05,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 1780708185545540736 20260416.4603 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.21,0.05,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 20260416.4603 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.4603 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.9603,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.4603 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
First image: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Last image: 2461146.96054875 16.04.2026 11:03:01.412 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
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: 5 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): 12615
Objects passed selection criteria: 12560
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 9758
Average stars matched: 8621.5 (88.3531 %)
Memory usage VmPeak: 116492 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 06:17:55 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: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
First image: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Last image: 2461146.96054875 16.04.2026 11:03:01.412 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 86
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 26 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 79233
Objects passed selection criteria: 78991
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 61512
Average stars matched: 54700 (88.9257 %)
Memory usage VmPeak: 173820 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 06:19:55 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/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461146.95998380
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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits exists and is non-empty
Saving wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits to local_wcs_cache/
'wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits' -> 'local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits'
wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits exists and is non-empty
Saving wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits to local_wcs_cache/
'wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits' -> 'local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:09:14.257 +21:59:49.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits (1st new image)
verification OK: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:08:59.872 +22:01:04.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:09:14.257 +21:59:49.67
Second-epoch image center 22:08:59.872 +22:01:04.89
Angular distance between the image centers 0.0594 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits (2nd new image)
verification OK: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:09:02.560 +22:01:04.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:09:14.257 +21:59:49.67
Second-epoch image center 22:09:02.560 +22:01:04.01
Angular distance between the image centers 0.0497 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 22:08:59.872 +22:01:04.89
Second-epoch second image center 22:09:02.560 +22:01:04.01
Angular distance between the image centers 0.01039 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/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.FKUmAOlYjy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.tD3WOyTiIZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits &> /tmp/tmp.Wiyc7AE1qz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits &> /tmp/tmp.HyAXxdrt9d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
The reference image (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits) and catalog (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat) found
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 12915 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 323.6044 to 341.1833 deg, Dec +16.4675 to +27.2977 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 323.6044 to 341.1833 deg, Dec 16.4675 to 27.2977 deg
Loaded 10718 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): 8028 out of 8532 total matches.
Matched with Tycho-2 8532 out of 12915 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.918847
a=0.000000 b=1.000000 c=22.918847
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.99
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
2.4 pix Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
2.8 pix fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
2.8 pix fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Limiting magnitude estimates:
15.0 mag. Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
15.0 mag. Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
14.8 mag. fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
14.7 mag. fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 12.0 (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.FKUmAOlYjy (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/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1046, passed=12915
Got 12915 stars (including 11858 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 12915 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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.tD3WOyTiIZ (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/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1022, passed=12932
Got 12932 stars (including 11893 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 12932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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.Wiyc7AE1qz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=933, passed=12114
Got 12114 stars (including 11177 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat
util/solve_plate_with_UCAC5 got 12114 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 11897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 11897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 11897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits -region wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.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.HyAXxdrt9d (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=935, passed=11989
Got 11989 stars (including 11046 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat
util/solve_plate_with_UCAC5 got 11989 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 532 to 588 (Dec 16.5 to 27.3)
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: 958 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 11739 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 532 to 588 (Dec 16.5 to 27.3)
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: 958 matched stars entering correct_measured_positions(), 11740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 11740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits -region wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
Saving fully-calibrated image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits'
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits'
Preparing the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out23358.dat to exclusion_list_apass.txt
make_report_in_HTML.sh Phase 1 (network queries): 46s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21827_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 21827_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:09:55.81 +18:47:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22697_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 22697_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:00:56.94 +21:33:44.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22768_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 22768_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:52:58.61 +23:12:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 1.252 1795045679733063040 328.24388410543 +23.21234609003 11.7863 11.0892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23352_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 23352_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:50:05.02 +20:48:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.954 1792624623847822848 327.52067373986 +20.81088669502 12.0538 11.5300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23358_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 23358_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:58:41.64 +21:34:51.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 46s
Prepared the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits exists and is non-empty
wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:09:14.257 +21:59:49.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits (1st new image)
verification OK: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:08:59.872 +22:01:04.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:09:14.257 +21:59:49.67
Second-epoch image center 22:08:59.872 +22:01:04.89
Angular distance between the image centers 0.0594 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits (2nd new image)
verification OK: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:09:02.560 +22:01:04.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:09:14.257 +21:59:49.67
Second-epoch image center 22:09:02.560 +22:01:04.01
Angular distance between the image centers 0.0497 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 22:08:59.872 +22:01:04.89
Second-epoch second image center 22:09:02.560 +22:01:04.01
Angular distance between the image centers 0.01039 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/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.xbLaV25oa3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.DK7bH2qNtZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits &> /tmp/tmp.5rjAmrSntY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits &> /tmp/tmp.6vU8iWIE0L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
The reference image (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits) and catalog (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat) found
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 86189 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 323.6044 to 341.2092 deg, Dec +16.4487 to +27.3003 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 323.6044 to 341.2092 deg, Dec 16.4487 to 27.3003 deg
Loaded 10750 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): 7498 out of 9018 total matches.
Matched with Tycho-2 9018 out of 86189 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.751336
a=0.000000 b=1.000000 c=22.751336
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 65 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
2.2 pix Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
2.6 pix fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
2.6 pix fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Limiting magnitude estimates:
15.2 mag. Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
15.2 mag. Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
14.8 mag. fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
14.8 mag. fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xbLaV25oa3 (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/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=6314, passed=86166
Got 86166 stars (including 79704 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 86166 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 532 to 588 (Dec 16.4 to 27.3)
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: 964 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 84836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
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: 964 matched stars entering correct_measured_positions(), 84836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 84836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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.DK7bH2qNtZ (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/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=6394, passed=85906
Got 85906 stars (including 79384 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 85906 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 962 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(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 84759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 962 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(), 84759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 84759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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.5rjAmrSntY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=5864, passed=65334
Got 65334 stars (including 59396 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat
util/solve_plate_with_UCAC5 got 65334 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 64204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 64204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 64204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits -region wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.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.6vU8iWIE0L (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=5820, passed=65053
Got 65053 stars (including 59167 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat
util/solve_plate_with_UCAC5 got 65053 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 63777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 63776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 63775 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits -region wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.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_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Saving fully-calibrated image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-02-12_20.00sec_-5.00C_LIGHT_0447.fits
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Peg-05-Q2b1x1_060349_TTUQ2b1x1_18141_1o2SWQrJ/wcs_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448.fits
Preparing the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out118015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out118660.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out119308.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out119608.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out101710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119123.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 782s
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: 38s
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Considering the candidate 101710_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101710_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101712_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101712_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101713_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101713_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101720_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101720_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101727_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101727_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 101730_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101730_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 101734_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101734_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 101740_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 101740_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:52:34.23 +22:03:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101741_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 101741_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 104786_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 104786_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:51:37.56 +19:56:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105112_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 105112_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:56:17.07 +22:52:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105403_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 105403_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:07:43.47 +21:41:17.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107231_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 107231_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 108104_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 108104_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:06:49.79 +25:51:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108359_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 108359_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:57:44.72 +23:42:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110983_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 110983_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:17:59.30 +24:09:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111119_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 111119_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:56:18.08 +22:30:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111260_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 111260_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 111326_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 111326_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:54:13.76 +21:45:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111522_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 111522_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:57:30.58 +23:33:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111986_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 111986_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:04:52.77 +21:16:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112197_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 112197_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:56:17.71 +18:19:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112285_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 112285_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 112493_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 112493_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:55:16.27 +23:59:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113879_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 113879_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:57:12.62 +24:31:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113976_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 113976_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:01:23.63 +24:17:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114479_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 114479_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114989_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 114989_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:09:58.97 +21:07:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115793_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 115793_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:07:01.77 +25:51:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116490_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 116490_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
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Considering the candidate 116583_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 116583_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116644_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 116644_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116803_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 116803_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116826_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 116826_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116953_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 116953_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117000_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 117000_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117040_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 117040_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117109_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 117109_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117302_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 117302_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117688_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 117688_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117817_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 117817_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117914_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 117914_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118015_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 118015_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:54:39.26 +20:43:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.086 1780947810361019392 328.66309190813 +20.72807528234 14.3531 13.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118660_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 118660_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:53:09.70 +17:57:03.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119123_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
Preparing report for the candidate 119123_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119296_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 119296_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:53:14.45 +24:20:39.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)
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Considering the candidate 119308_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 119308_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:03:25.54 +25:23:46.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)
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Considering the candidate 119390_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 119390_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:04:11.29 +24:37:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.270 1795470812776831616 331.04689047717 +24.62929712819 14.8094 14.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119563_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 119563_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:52:14.82 +21:51:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 3.242 1793210045070064256 328.06181942412 +21.85198146124 14.8654 14.3427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119608_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 119608_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:52:01.82 +24:48:34.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.67, MAG_FAINT_SEARCH_LIMIT=15.65)
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Considering the candidate 119715_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 119715_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:50:47.56 +24:08:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 2.074 1795919619678323584 327.69755531075 +24.14836600647 14.6655 14.2096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119891_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 119891_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:54:23.36 +19:48:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 2.935 1780306382765201664 328.59647741997 +19.80123890349 14.8550 14.2503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120140_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120140_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:55:40.86 +23:05:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.130 1794815057169003648 328.91992743690 +23.08346337973 14.5554 13.5840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120239_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120239_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:03:43.97 +23:10:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 0.728 1783217477238491264 330.93311373389 +23.16723807970 14.8017 13.9818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120260_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120260_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:05:51.06 +25:05:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 0.674 1891586855101852800 331.46254379144 +25.08654228888 14.9281 14.3629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120290_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120290_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:56:55.46 +24:46:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.474 1795625603397816576 329.23094749359 +24.77862913386 14.7115 14.1973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120341_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120341_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:54:55.49 +22:52:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.623 1794787947335425664 328.73075833901 +22.86915616229 14.7996 14.2618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120425_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120425_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:02:11.27 +23:29:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.439 1795251322767104640 330.54695247322 +23.49720517126 14.5229 13.9154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120527_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120527_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:05:43.49 +22:33:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.883 1782939335156356352 331.43099676111 +22.55917611502 14.5495 13.7851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120557_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120557_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 21:57:01.26 +21:15:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.528 1781085833430109824 329.25479484058 +21.25314279792 15.1345 14.5356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120599_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120599_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:08:05.44 +25:48:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 3.783 1891740821089049984 332.02160963125 +25.81089041765 14.5662 14.0287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120772_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 120772_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:12:47.81 +22:02:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 1.845 1782065910607079424 333.19869573683 +22.03714134755 14.7262 14.2096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70393_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 70393_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:09:55.82 +18:47:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50256_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 50256_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:00:56.98 +21:33:44.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09608_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448
The candidate 09608_fd_Peg-05-Q2b1x1_2026-04-16_06-03-01_20.00sec_-4.90C_LIGHT_0448 did not pass the final checks
**** FOUND 22:05:10.76 +26:14:39.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 825s
Prepared the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:08:42.80 +20:26:10.9
21:55:03.50 +23:33:58.3
22:09:31.65 +24:08:51.4
22:08:53.33 +21:51:27.5
21:53:08.89 +25:15:59.9
21:59:00.20 +22:56:42.6
22:02:02.78 +25:28:45.1
21:49:47.43 +25:56:25.2
21:50:32.35 +25:01:09.6
21:58:29.87 +23:04:12.2
21:54:51.50 +25:44:45.7
21:54:13.78 +24:47:06.0
22:02:32.07 +26:11:14.0
21:54:58.89 +22:58:51.0
21:49:48.60 +23:22:35.0
22:03:46.69 +20:25:29.6
21:50:08.87 +18:19:53.5
21:53:27.31 +24:40:14.6
21:54:01.75 +23:22:02.6
21:51:48.20 +22:48:24.7
22:05:24.85 +25:51:21.6
21:53:46.91 +22:14:00.8
21:55:13.01 +20:10:31.5
22:01:29.75 +18:20:55.5
21:54:54.18 +24:25:35.6
21:59:48.44 +20:23:08.5
########### Completed Peg-05-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 ####
22:08:42.80 +20:26:10.9
21:55:03.50 +23:33:58.3
22:09:31.65 +24:08:51.4
22:08:53.33 +21:51:27.5
21:53:08.89 +25:15:59.9
21:59:00.20 +22:56:42.6
22:02:02.78 +25:28:45.1
21:49:47.43 +25:56:25.2
21:50:32.35 +25:01:09.6
21:58:29.87 +23:04:12.2
21:54:51.50 +25:44:45.7
21:54:13.78 +24:47:06.0
22:02:32.07 +26:11:14.0
21:54:58.89 +22:58:51.0
21:49:48.60 +23:22:35.0
22:03:46.69 +20:25:29.6
21:50:08.87 +18:19:53.5
21:53:27.31 +24:40:14.6
21:54:01.75 +23:22:02.6
21:51:48.20 +22:48:24.7
22:05:24.85 +25:51:21.6
21:53:46.91 +22:14:00.8
21:55:13.01 +20:10:31.5
22:01:29.75 +18:20:55.5
21:54:54.18 +24:25:35.6
21:59:48.44 +20:23:08.5
###################################################################################
22:08:42.80 +20:26:10.9 -- not an asteroid (will add it to exclusion list)
21:55:03.50 +23:33:58.3 -- not an asteroid (will add it to exclusion list)
22:09:31.65 +24:08:51.4 -- not an asteroid (will add it to exclusion list)
22:08:53.33 +21:51:27.5 -- not an asteroid (will add it to exclusion list)
21:53:08.89 +25:15:59.9 -- not an asteroid (will add it to exclusion list)
21:59:00.20 +22:56:42.6 -- not an asteroid (will add it to exclusion list)
22:02:02.78 +25:28:45.1 -- not an asteroid (will add it to exclusion list)
21:49:47.43 +25:56:25.2 -- not an asteroid (will add it to exclusion list)
21:50:32.35 +25:01:09.6 -- not an asteroid (will add it to exclusion list)
21:58:29.87 +23:04:12.2 -- not an asteroid (will add it to exclusion list)
21:54:51.50 +25:44:45.7 -- not an asteroid (will add it to exclusion list)
21:54:13.78 +24:47:06.0 -- not an asteroid (will add it to exclusion list)
22:02:32.07 +26:11:14.0 -- not an asteroid (will add it to exclusion list)
21:54:58.89 +22:58:51.0 -- not an asteroid (will add it to exclusion list)
21:49:48.60 +23:22:35.0 -- not an asteroid (will add it to exclusion list)
22:03:46.69 +20:25:29.6 -- not an asteroid (will add it to exclusion list)
21:50:08.87 +18:19:53.5 -- not an asteroid (will add it to exclusion list)
21:53:27.31 +24:40:14.6 -- not an asteroid (will add it to exclusion list)
21:54:01.75 +23:22:02.6 -- not an asteroid (will add it to exclusion list)
21:51:48.20 +22:48:24.7 -- not an asteroid (will add it to exclusion list)
22:05:24.85 +25:51:21.6 -- not an asteroid (will add it to exclusion list)
21:53:46.91 +22:14:00.8 -- not an asteroid (will add it to exclusion list)
21:55:13.01 +20:10:31.5 -- not an asteroid (will add it to exclusion list)
22:01:29.75 +18:20:55.5 -- not an asteroid (will add it to exclusion list)
21:54:54.18 +24:25:35.6 -- not an asteroid (will add it to exclusion list)
21:59:48.44 +20:23:08.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:49:47.43 +25:56:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:48.60 +23:22:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:08.87 +18:19:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:32.35 +25:01:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:48.20 +22:48:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:08.89 +25:15:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:27.31 +24:40:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:46.91 +22:14:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:01.75 +23:22:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:13.78 +24:47:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:51.50 +25:44:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:54.18 +24:25:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:58.89 +22:58:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:03.50 +23:33:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:13.01 +20:10:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:29.87 +23:04:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:00.20 +22:56:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:48.44 +20:23:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:29.75 +18:20:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:02.78 +25:28:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:32.07 +26:11:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:46.69 +20:25:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:24.85 +25:51:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:42.80 +20:26:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:53.33 +21:51:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:31.65 +24:08:51.4 -- 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)
21:49:47.43 +25:56:25.2 -- not a known variable star
21:49:48.60 +23:22:35.0 -- not a known variable star
21:50:08.87 +18:19:53.5 -- not a known variable star
21:50:32.35 +25:01:09.6 -- not a known variable star
21:51:48.20 +22:48:24.7 -- not a known variable star
21:53:08.89 +25:15:59.9 -- a known variable star
21:53:27.31 +24:40:14.6 -- not a known variable star
21:53:46.91 +22:14:00.8 -- not a known variable star
21:54:01.75 +23:22:02.6 -- not a known variable star
21:54:13.78 +24:47:06.0 -- not a known variable star
21:54:51.50 +25:44:45.7 -- not a known variable star
21:54:54.18 +24:25:35.6 -- not a known variable star
21:54:58.89 +22:58:51.0 -- not a known variable star
21:55:03.50 +23:33:58.3 -- not a known variable star
21:55:13.01 +20:10:31.5 -- not a known variable star
21:58:29.87 +23:04:12.2 -- not a known variable star
21:59:00.20 +22:56:42.6 -- not a known variable star
21:59:48.44 +20:23:08.5 -- not a known variable star
22:01:29.75 +18:20:55.5 -- not a known variable star
22:02:02.78 +25:28:45.1 -- not a known variable star
22:02:32.07 +26:11:14.0 -- not a known variable star
22:03:46.69 +20:25:29.6 -- a known variable star
22:05:24.85 +25:51:21.6 -- not a known variable star
22:08:42.80 +20:26:10.9 -- not a known variable star
22:08:53.33 +21:51:27.5 -- not a known variable star
22:09:31.65 +24:08:51.4 -- not a known variable star
Found 24 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
26 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
21:49:47.43 +25:56:25.2
21:49:48.60 +23:22:35.0
21:50:08.87 +18:19:53.5
21:50:32.35 +25:01:09.6
21:51:48.20 +22:48:24.7
21:53:08.89 +25:15:59.9
21:53:27.31 +24:40:14.6
21:53:46.91 +22:14:00.8
21:54:01.75 +23:22:02.6
21:54:13.78 +24:47:06.0
21:54:51.50 +25:44:45.7
21:54:54.18 +24:25:35.6
21:54:58.89 +22:58:51.0
21:55:03.50 +23:33:58.3
21:55:13.01 +20:10:31.5
21:58:29.87 +23:04:12.2
21:59:00.20 +22:56:42.6
21:59:48.44 +20:23:08.5
22:01:29.75 +18:20:55.5
22:02:02.78 +25:28:45.1
22:02:32.07 +26:11:14.0
22:03:46.69 +20:25:29.6
22:05:24.85 +25:51:21.6
22:08:42.80 +20:26:10.9
22:08:53.33 +21:51:27.5
22:09:31.65 +24:08:51.4
21:52:58.61 +23:12:43.8
21:50:05.02 +20:48:38.7
21:54:39.26 +20:43:39.8
21:53:14.45 +24:20:39.7
22:04:11.29 +24:37:44.3
21:52:14.82 +21:51:03.9
21:50:47.56 +24:08:53.6
21:54:23.36 +19:48:04.0
21:55:40.86 +23:05:00.1
22:03:43.97 +23:10:01.4
22:05:51.06 +25:05:11.5
21:56:55.46 +24:46:42.9
21:54:55.49 +22:52:09.6
22:02:11.27 +23:29:49.5
22:05:43.49 +22:33:32.5
21:57:01.26 +21:15:09.3
22:08:05.44 +25:48:37.6
22:12:47.81 +22:02:14.4
21:58:41.64 +21:34:51.4
21:53:09.70 +17:57:03.1
22:03:25.54 +25:23:46.5
21:52:01.82 +24:48:34.1
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461146.95998380 -observatory V36
00:09:44.10 -01:48:13.9 Mercury (0.0mag)
03:10:54.25 +18:01:44.9 Venus (-3.9mag)
00:19:09.17 +01:00:30.7 Mars (1.2mag)
07:12:50.43 +22:45:52.4 Jupiter (-2.1mag)
00:29:23.24 +00:50:15.4 Saturn (0.9mag)
03:47:47.66 +19:47:47.0 Uranus (5.8mag)
00:10:54.05 -00:14:59.6 Neptune (7.8mag)
20:33:46.50 -22:52:37.3 Pluto (14.5mag)
00:43:02.37 +06:52:35.2 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Apr 16 06:17 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461146.95998380:
07:12:58.30 +22:45:36.5 Io (5.8mag)
07:13:01.38 +22:45:30.5 Europa (5.9mag)
07:13:03.57 +22:45:19.4 Ganymede (5.4mag)
07:13:25.61 +22:44:39.2 Callisto (6.6mag)
07:16:09.48 +22:33:17.2 Himalia (15.3mag)
07:12:53.06 +22:45:48.5 Thebe (16.2mag)
07:16:21.46 +23:03:30.6 Elara (17.3mag)
07:11:45.23 +23:25:38.2 Pasiphae (17.4mag)
07:21:09.55 +22:43:56.4 Carme (18.5mag)
00:29:22.37 +00:50:42.6 Titan (8.8mag)
00:29:23.73 +00:50:16.3 Rhea (10.1mag)
00:29:02.47 +00:50:20.4 Iapetus (11.5mag)
00:29:29.90 +00:50:37.3 Hyperion (14.8mag)
00:30:59.76 +00:59:00.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 16 06:18 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461146.95998380:
15:39:11.29 -16:36:47.0 JWST
15:33:45.23 +52:31:22.7 Chandra
09:12:22.24 -52:33:18.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 16 06:17 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461146.95998380 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:11.22 -28:48:23.4 13.9mag P/2010 H2 (Vales)
05:07:04.07 -69:38:24.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:32.82 +31:26:25.5 17.2mag C/2017 K2 (PANSTARRS)
17:30:23.28 +10:36:07.7 17.6mag C/2021 G2 (ATLAS)
23:10:20.81 +29:14:50.4 17.1mag C/2022 E2 (ATLAS)
04:29:46.49 +26:03:02.6 16.0mag C/2022 N2 (PANSTARRS)
09:03:31.20 +32:01:11.7 16.2mag C/2022 QE78 (ATLAS)
08:31:08.70 -00:06:16.6 17.3mag C/2022 R6 (PANSTARRS)
18:53:37.22 +18:34:15.8 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:31.36 -11:30:53.6 17.5mag P/2023 B1 (PANSTARRS)
09:07:25.47 -11:48:34.7 17.6mag C/2023 F3 (ATLAS)
21:54:40.57 +62:56:01.8 17.5mag C/2023 H5 (Lemmon)
19:18:47.79 -03:44:25.1 14.1mag C/2023 R1 (PANSTARRS)
21:31:35.22 +85:58:33.0 17.8mag C/2023 X2 (Lemmon)
06:18:07.09 +63:30:38.0 17.2mag C/2024 A1 (ATLAS)
05:14:15.76 +18:27:34.0 11.1mag C/2024 E1 (Wierzchos)
16:18:58.64 +06:27:56.9 17.4mag C/2024 G6 (ATLAS)
20:20:56.33 +15:23:59.0 14.6mag C/2024 J3 (ATLAS)
03:26:47.05 -22:18:56.3 16.3mag C/2024 T5 (ATLAS)
05:17:06.38 +45:10:36.9 17.7mag C/2025 J1 (Borisov)
13:36:54.86 +45:47:04.5 15.2mag C/2025 L1 (ATLAS)
03:26:00.53 -26:17:01.1 17.8mag C/2025 Q3 (ATLAS)
23:47:38.76 +18:26:43.7 8.4mag C/2025 R3 (PANSTARRS)
12:53:55.03 +03:02:26.2 17.4mag C/2025 Y1 (ATLAS)
03:31:39.16 +02:34:19.5 13.4mag C/2026 A1 (MAPS)
00:00:53.15 +37:18:13.8 14.6mag C/2026 B2 (Sun-Gao)
18:43:49.64 -09:41:41.1 11.8mag 10P/Tempel
14:59:40.02 +03:09:39.7 14.0mag 24P/Schaumasse
11:02:40.77 -01:30:41.2 15.7mag 29P/Schwassmann-Wachmann
18:01:05.22 -09:35:36.9 18.0mag 40P/Vaisala
10:37:32.76 -04:03:45.4 16.9mag 43P/Wolf-Harrington
01:49:23.33 +17:33:57.4 17.2mag 47P/Ashbrook-Jackson
07:11:37.02 +36:54:46.7 17.0mag 63P/Wild
23:29:38.71 -11:23:45.0 15.7mag 65P/Gunn
04:04:29.13 +21:24:44.0 15.9mag 76P/West-Kohoutek-Ikemura
01:06:35.79 +08:19:08.5 14.3mag 78P/Gehrels
23:04:23.84 -09:15:18.8 14.6mag 88P/Howell
02:11:42.54 +20:45:52.4 15.1mag 93P/Lovas
04:55:40.57 +32:18:42.3 16.2mag 123P/West-Hartley
08:28:54.37 +38:08:52.0 16.2mag 124P/Mrkos
02:33:55.81 +14:25:16.3 16.4mag 128P/Shoemaker-Holt
02:48:26.61 +14:32:56.6 17.5mag 131P/Mueller
01:28:35.60 +13:23:46.5 10.6mag 141P/Machholz
01:37:27.41 +05:02:46.5 10.6mag 141P-A/Machholz
00:22:31.99 +00:56:21.8 12.8mag 141P-D/Machholz
02:07:49.31 +06:48:20.6 17.8mag 141P-I/Machholz
01:03:40.02 -01:17:39.2 15.1mag 162P/SidingSpring
14:50:36.49 -00:01:16.1 17.7mag 210P/Christensen
21:40:10.48 -11:20:17.6 17.6mag 218P/LINEAR
17:16:40.26 -13:52:41.5 16.1mag 235P/LINEAR
05:35:28.82 +34:43:58.0 16.8mag 240P/NEAT
07:38:43.33 -05:07:03.2 17.7mag 242P/Spahr
22:18:03.71 -20:51:26.9 17.9mag 260P/McNaught
01:59:07.95 +20:34:34.1 18.0mag 295P/LINEAR
15:42:27.73 +07:01:14.5 17.5mag 391P/Kowalski
07:34:22.48 +21:22:01.8 17.7mag 450P/LONEOS
05:36:32.72 +45:00:19.4 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 16 06:17 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
15:25:54.99 +07:49:24.50 2026-04-12.14 16.96
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
-rw-r--r-- 1 apache apache 5.8K Apr 16 06:17 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 16 06:17 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:32:40.720 +02:42:54.71 AT 2026jay 2026-04-06.66 22
14:07:18.110 +04:13:29.83 AT 2026jax 2026-04-06.66 22.26
14:14:08.750 +03:35:26.74 AT 2026jaw 2026-04-06.66 22.24
14:03:53.740 +04:33:03.03 AT 2026jav 2026-04-06.66 22.18
14:07:43.620 +03:35:48.12 AT 2026jau 2026-04-06.66 21.82
14:10:23.930 -01:02:22.49 AT 2026jat 2026-04-06.65 22.15
13:51:42.460 +03:14:48.63 AT 2026jas 2026-04-06.65 21.87
13:42:53.750 +01:22:24.17 AT 2026jar 2026-04-06.65 22.6
13:44:21.040 -01:54:42.32 AT 2026jaq 2026-04-06.65 22.71
13:35:29.290 +00:58:49.10 AT 2026jap 2026-04-06.64 22.39
13:41:45.110 +04:07:23.04 AT 2026jao 2026-04-06.64 21.84
13:38:11.980 +03:37:12.11 AT 2026jan 2026-04-06.64 22.48
13:27:27.970 +05:34:49.94 AT 2026jam 2026-04-06.64 21.79
13:28:44.170 +03:09:01.26 AT 2026jal 2026-04-06.64 22.01
13:29:02.030 -02:11:15.98 AT 2026jak 2026-04-06.64 21.54
13:11:37.460 +01:53:43.84 AT 2026jaj 2026-04-06.63 21.95
13:13:23.110 +00:38:42.68 AT 2026jai 2026-04-06.63 21.88
13:19:01.640 +03:04:08.10 AT 2026jah 2026-04-06.63 22.02
13:06:29.860 +02:34:35.75 AT 2026jag 2026-04-06.63 22.28
13:04:16.080 -00:23:58.35 AT 2026jaf 2026-04-06.63 22.55
-rw-r--r-- 1 apache apache 30K Apr 16 06:17 tns_transients_list.txt
