This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF
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
NSV 1469,2461144.7217,10.21,0.05,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
NSV 1469 20260414.2217 10.21CV 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
GSC 04336-02265,2461144.7217,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 04336-02265 20260414.2217 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0356573+703428,2461144.7217,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0356573+703428 20260414.2217 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496676580820098560,2461144.7217,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496676580820098560 20260414.2217 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.7217,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2217 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.7217,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2217 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.7217,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.2217 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GV Cam,2461144.7217,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GV Cam 20260414.2217 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J040808.04+655554.9,2461144.7217,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J040808.04+655554.9 20260414.2217 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0431018+693638,2461144.7217,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0431018+693638 20260414.2217 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 514871,2461144.7217,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 514871 20260414.2217 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0442135+724552,2461144.7217,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0442135+724552 20260414.2217 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0405390+661955,2461144.7217,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0405390+661955 20260414.2217 12.27CV 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
NSVS J0444316+724835,2461144.7217,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0444316+724835 20260414.2217 11.90CV 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
ZTF J043349.29+662343.6,2461144.7217,13.10,0.05,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
ZTF J043349.29+662343.6 20260414.2217 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0351564+725017,2461144.7217,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0351564+725017 20260414.2217 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050256.72+730320.7,2461144.7217,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050256.72+730320.7 20260414.2217 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
First image: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Last image: 2461144.72203802 14.04.2026 05:19:34.085 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 13353
Objects passed selection criteria: 13311
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 10807.5
Average stars matched: 10431.5 (96.5209 %)
Memory usage VmPeak: 119220 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 00:21:43 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
First image: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Last image: 2461144.72203802 14.04.2026 05:19:34.085 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 77
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 22 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): 93287
Objects passed selection criteria: 93057
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 70813.2
Average stars matched: 67998.8 (96.0255 %)
Memory usage VmPeak: 1930944 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 00:23:15 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461144.72134627
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits'
wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:16.792 +69:58:46.61
Second-epoch image center 04:47:59.492 +70:00:24.28
Angular distance between the image centers 0.0666 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:16.792 +69:58:46.61
Second-epoch image center 04:47:58.352 +69:59:47.41
Angular distance between the image centers 0.0616 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 04:47:59.492 +70:00:24.28
Second-epoch second image center 04:47:58.352 +69:59:47.41
Angular distance between the image centers 0.01037 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits &> /tmp/tmp.OkI6Eo2Zvd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits &> /tmp/tmp.bygIka6zM6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits &> /tmp/tmp.F78C5ambOa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits &> /tmp/tmp.dS9EwiMfLV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits) and catalog (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat) found
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat' -> 'wcsmag.cat'
Read 17535 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 44.4953 to 100.0749 deg, Dec +62.8164 to +75.4615 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 44.4953 to 100.0749 deg, Dec 62.8164 to 75.4615 deg
Loaded 14408 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): 7701 out of 8346 total matches.
Matched with Tycho-2 8346 out of 17535 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.930229
a=0.000000 b=1.000000 c=22.930229
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
2.0 pix Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
3.2 pix fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
3.2 pix fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Limiting magnitude estimates:
15.4 mag. Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
15.4 mag. Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
14.4 mag. fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
14.3 mag. fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OkI6Eo2Zvd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1440, passed=17535
Got 17535 stars (including 16074 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 17535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 17045 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 17045 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 17045 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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.bygIka6zM6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1424, passed=17523
Got 17523 stars (including 16079 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 17523 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 17070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 17071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 17071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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.F78C5ambOa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=653, passed=9268
Got 9268 stars (including 8613 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat
util/solve_plate_with_UCAC5 got 9268 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 966 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(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 966 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(), 9020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
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_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits -region wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.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.dS9EwiMfLV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=699, passed=9116
Got 9116 stars (including 8413 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat
util/solve_plate_with_UCAC5 got 9116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 768 to 828 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 966 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(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 8849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 966 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(), 8848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 8848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
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_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits -region wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits'
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out06784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11072.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21051_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 21051_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:40:17.07 +66:08:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 2.670 483143555486324992 070.07160299110 +66.13472833216 9.6439 8.3302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21188_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 21188_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:18:00.82 +71:13:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14398_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 14398_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:54:02.81 +66:20:40.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11072_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 11072_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06784_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 06784_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07990_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 07990_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05376_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 05376_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:13:45.18 +72:07:33.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11005_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 11005_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:06:03.62 +68:40:49.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cam-06-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 ####
04:22:57.24 +71:18:48.5
03:56:58.27 +70:34:27.7
04:10:17.32 +68:42:07.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:16.792 +69:58:46.61
Second-epoch image center 04:47:59.492 +70:00:24.28
Angular distance between the image centers 0.0666 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:16.792 +69:58:46.61
Second-epoch image center 04:47:58.352 +69:59:47.41
Angular distance between the image centers 0.0616 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 04:47:59.492 +70:00:24.28
Second-epoch second image center 04:47:58.352 +69:59:47.41
Angular distance between the image centers 0.01037 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits &> /tmp/tmp.NwlvBeCVKa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits &> /tmp/tmp.gqtAsOaoQo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits &> /tmp/tmp.w4gPAYmLtL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits &> /tmp/tmp.7fgyKclsPA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits) and catalog (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat) found
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat' -> 'wcsmag.cat'
Read 121322 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 44.3972 to 100.3253 deg, Dec +62.8165 to +75.4640 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 44.3972 to 100.3253 deg, Dec 62.8165 to 75.4640 deg
Loaded 14499 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): 6542 out of 8413 total matches.
Matched with Tycho-2 8413 out of 121322 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.798908
a=0.000000 b=1.000000 c=22.798908
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 61 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
1.9 pix Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
3.1 pix fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
3.2 pix fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Limiting magnitude estimates:
15.6 mag. Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
15.6 mag. Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
14.5 mag. fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
14.5 mag. fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.8 (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.NwlvBeCVKa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=10875, passed=121302
Got 121302 stars (including 110227 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 121302 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 118877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 118876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 118876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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.gqtAsOaoQo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=10830, passed=121526
Got 121526 stars (including 110505 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 121526 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 119031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 119030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 119030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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.w4gPAYmLtL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=4135, passed=48295
Got 48295 stars (including 44117 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat
util/solve_plate_with_UCAC5 got 48295 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 961 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(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 47205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 961 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(), 47207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 47207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits -region wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.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.7fgyKclsPA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3968, passed=46646
Got 46646 stars (including 42632 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat
util/solve_plate_with_UCAC5 got 46646 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 768 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 961 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(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 45263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 768 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 961 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(), 45263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 45263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits -region wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-18-34_20.00sec_-5.00C_LIGHT_0791.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cam-06-Q2b1x1_002027_TTUQ2b1x1_25527_4878hZCF/wcs_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792.fits
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out140088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out140099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99603.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 140088_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140088_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:11:57.98 +66:28:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.506 489570888144900352 062.99408523343 +66.47024148571 13.2969 12.5424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140092_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140092_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:23:42.00 +66:24:56.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 140096_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140096_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:46:30.28 +65:37:08.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 140098_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140098_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:11:46.45 +68:02:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.142 490753103662710400 062.94044940811 +68.03694936058 13.4667 12.7830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140099_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 140099_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 140101_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 140101_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 140103_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140103_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:21:28.87 +68:10:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.784 490539420449265664 065.37384104836 +68.17548986933 13.1667 12.5408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140105_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140105_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:15:50.99 +65:54:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 140106_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 140106_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 140107_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140107_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 03:58:20.45 +73:31:37.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)
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Considering the candidate 140113_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140113_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:02:20.28 +72:25:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140250_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140250_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:40:17.09 +66:08:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)GAIADR2_OUTPUT=# 2.349 483143555486324992 070.07160299110 +66.13472833216 9.6439 8.3302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140709_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140709_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:17:16.34 +66:57:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140910_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 140910_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:03:07.64 +66:49:10.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141045_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141045_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:59:57.62 +70:27:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141054_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141054_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:50:06.05 +66:30:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141070_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141070_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:51:32.46 +68:11:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141080_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141080_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:51:33.93 +68:12:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141103_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141103_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:13:20.16 +72:06:35.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141269_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141269_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:13:53.91 +67:29:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141370_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141370_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:37:29.11 +66:41:32.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141402_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141402_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:13:40.91 +72:09:22.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141434_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141434_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:02:58.48 +72:49:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141494_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141494_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:02:40.36 +66:48:10.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141540_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 141540_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 141586_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141586_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:42:47.94 +71:16:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141630_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141630_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:21:53.79 +67:02:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141669_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141669_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:22:34.99 +67:04:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141696_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141696_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:20:28.60 +71:45:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141705_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141705_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:09:46.25 +68:22:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141787_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141787_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:14:25.22 +69:50:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141886_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 141886_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:26:31.32 +70:13:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142267_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 142267_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:22:21.54 +65:57:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.947 489352050971194368 065.58970917263 +65.95898736608 12.9446 11.3719 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99603_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 99603_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 91484_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 91484_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 66572_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 66572_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 57897_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 57897_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 45101_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 45101_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:22:57.26 +71:18:48.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 26591_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 26591_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 54084_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 54084_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 03:56:58.30 +70:34:27.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 55699_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 55699_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:14:19.79 +69:51:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46725_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 46725_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:18:00.73 +71:13:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96064_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 96064_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 25862_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 25862_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 120725_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 120725_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:10:17.16 +68:42:06.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 66789_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 66789_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:37:48.87 +69:31:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98220_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 98220_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 26141_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 26141_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 20853_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
Preparing report for the candidate 20853_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
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Considering the candidate 46440_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 46440_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:50:36.33 +70:56:28.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67437_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 67437_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:29:52.20 +69:22:42.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 118219_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 118219_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:51:13.16 +68:10:11.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 28881_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 28881_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:33:30.90 +72:31:39.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118723_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 118723_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:12:51.66 +68:30:04.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33229_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 33229_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:13:45.16 +72:07:32.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 26825_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 26825_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 03:58:02.72 +72:43:28.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 85083_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 85083_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:06:03.62 +68:40:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 100036_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 100036_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 04:54:02.81 +66:20:40.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 11647_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 11647_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 05:04:12.45 +73:45:47.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 37055_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 37055_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
**** FOUND 03:56:29.74 +71:49:18.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 08879_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792
The candidate 08879_fd_Cam-06-Q2b1x1_2026-04-14_00-19-34_20.00sec_-5.00C_LIGHT_0792 did not pass the final checks
