This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc
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
ATO J312.4898+47.5687,2461144.8096,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.4898+47.5687 20260414.3096 12.13CV 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 J203618.10+500035.5,2461144.8096,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203618.10+500035.5 20260414.3096 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2013354+421223,2461144.8096,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2013354+421223 20260414.3096 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203448.56+460517.9,2461144.8096,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J203448.56+460517.9 20260414.3096 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203449.49+482346.0,2461144.8096,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203449.49+482346.0 20260414.3096 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.5692+48.3173,2461144.8096,12.10,0.05,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
ATO J310.5692+48.3173 20260414.3096 12.10CV 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
ATO J311.5801+44.9420,2461144.8096,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.5801+44.9420 20260414.3096 11.79CV 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 J202846.83+494233.3,2461144.8096,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J202846.83+494233.3 20260414.3096 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5787193,2461144.8096,10.81,0.05,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 5787193 20260414.3096 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202918.68+500641.3,2461144.8096,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202918.68+500641.3 20260414.3096 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J204610.23+441045.3,2461144.8096,10.76,0.05,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 J204610.23+441045.3 20260414.3096 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168151859570189696,2461144.8096,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168151859570189696 20260414.3096 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0514 Cyg,2461144.8096,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0514 Cyg 20260414.3096 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203452.37+472937.4,2461144.8096,12.10,0.05,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
ASASSN-V J203452.37+472937.4 20260414.3096 12.10CV 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
ASASSN-V J203945.88+474117.1,2461144.8096,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203945.88+474117.1 20260414.3096 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201925.38+420132.2,2461144.8096,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201925.38+420132.2 20260414.3096 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204508.26+453924.1,2461144.8096,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204508.26+453924.1 20260414.3096 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2032 Cyg,2461144.8096,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2032 Cyg 20260414.3096 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202057.62+495828.7,2461144.8096,12.17,0.05,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 J202057.62+495828.7 20260414.3096 12.17CV 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 2087447568640663168,2461144.8096,12.63,0.05,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 2087447568640663168 20260414.3096 12.63CV 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 J204822.11+492456.9,2461144.8096,11.53,0.05,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 J204822.11+492456.9 20260414.3096 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
First image: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Last image: 2461144.80986027 14.04.2026 07:26:01.927 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.04
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 21620
Objects passed selection criteria: 21468
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 13529.5
Average stars matched: 12567.5 (92.8896 %)
Memory usage VmPeak: 126060 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 02:28:28 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
First image: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Last image: 2461144.80986027 14.04.2026 07:26:01.927 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 161
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 34 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): 155815
Objects passed selection criteria: 155283
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 101645
Average stars matched: 93364.2 (91.8535 %)
Memory usage VmPeak: 2244252 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 02:31:45 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/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat to cache
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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: 2461144.80927476
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits exists and is non-empty
Saving wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits to local_wcs_cache/
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> 'local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits exists and is non-empty
Saving wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits to local_wcs_cache/
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> 'local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits exists and is non-empty
Saving wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits to local_wcs_cache/
'wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits' -> 'local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits'
wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits exists and is non-empty
Saving wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits to local_wcs_cache/
'wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits' -> 'local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:49.887 +46:01:07.95
Angular distance between the image centers 0.0380 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 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:49.232 +46:01:11.06
Angular distance between the image centers 0.0401 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 20:23:49.887 +46:01:07.95
Second-epoch second image center 20:23:49.232 +46:01:11.06
Angular distance between the image centers 0.00208 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/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits &> /tmp/tmp.kdHJQYFCE9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits &> /tmp/tmp.8uAQEf2sbw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits &> /tmp/tmp.pOg9aZWdAZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits &> /tmp/tmp.v8Fc6kXzZN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
The reference image (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits) and catalog (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat) found
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat' -> 'wcsmag.cat'
Read 27960 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 293.9748 to 318.5834 deg, Dec +39.9649 to +51.3609 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 293.9748 to 318.5834 deg, Dec 39.9649 to 51.3609 deg
Loaded 24546 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): 15113 out of 16730 total matches.
Matched with Tycho-2 16730 out of 27960 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914223
a=0.000000 b=1.000000 c=22.914223
From vast_summary.log: estimated ref. image limiting mag.: -8.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.87
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.87
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
2.4 pix Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
3.0 pix fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
2.9 pix fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Limiting magnitude estimates:
14.9 mag. Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
14.9 mag. Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
12.8 mag. fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
12.7 mag. fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.kdHJQYFCE9 (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/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3305, passed=27960
Got 27960 stars (including 24617 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 27960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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.8uAQEf2sbw (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/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3383, passed=28049
Got 28049 stars (including 24641 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 28049 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 26905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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.pOg9aZWdAZ (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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=366, passed=7436
Got 7436 stars (including 7064 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat
util/solve_plate_with_UCAC5 got 7436 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 7281 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 7280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 7280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.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.v8Fc6kXzZN (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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=331, passed=7107
Got 7107 stars (including 6770 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat
util/solve_plate_with_UCAC5 got 7107 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 6962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 6962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 6962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
Saving fully-calibrated image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits'
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits'
Preparing the HTML report for the field Cyg-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22617_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 22617_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:45:13.72 +42:20:09.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03063_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 03063_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:01:27.71 +50:02:29.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15197_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 15197_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:41:25.33 +45:16:50.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12772_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 12772_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:48:56.18 +46:06:51.5 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cyg-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat to cache
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Creating symlink local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits exists and is non-empty
wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits exists and is non-empty
wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits exists and is non-empty
wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:49.887 +46:01:07.95
Angular distance between the image centers 0.0380 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 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:49.232 +46:01:11.06
Angular distance between the image centers 0.0401 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 20:23:49.887 +46:01:07.95
Second-epoch second image center 20:23:49.232 +46:01:11.06
Angular distance between the image centers 0.00208 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/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits &> /tmp/tmp.ywWRv8Dhsj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits &> /tmp/tmp.mLOby7ssku
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits &> /tmp/tmp.KIQRW5qeY5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits &> /tmp/tmp.SOHNyG4a2t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
The reference image (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits) and catalog (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat) found
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat' -> 'wcsmag.cat'
Read 199760 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 293.9597 to 318.6913 deg, Dec +39.8908 to +51.3610 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 293.9597 to 318.6913 deg, Dec 39.8908 to 51.3610 deg
Loaded 24876 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): 12274 out of 18412 total matches.
Matched with Tycho-2 18412 out of 199760 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.735380
a=0.000000 b=1.000000 c=22.735380
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 116 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
2.2 pix Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
2.7 pix fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
2.7 pix fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Limiting magnitude estimates:
15.0 mag. Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
15.0 mag. Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
13.1 mag. fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
13.1 mag. fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.7 (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.ywWRv8Dhsj (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/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=32550, passed=199702
Got 199702 stars (including 166829 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 199702 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 193921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 193921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 193921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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.mLOby7ssku (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/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=32762, passed=199652
Got 199652 stars (including 166589 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 199652 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 194410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 194410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 194410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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.KIQRW5qeY5 (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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3565, passed=55383
Got 55383 stars (including 51744 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat
util/solve_plate_with_UCAC5 got 55383 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 54421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 54421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 54421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.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.SOHNyG4a2t (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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3327, passed=52792
Got 52792 stars (including 49413 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat
util/solve_plate_with_UCAC5 got 52792 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 51945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 51946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 51946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-14_CI_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Saving fully-calibrated image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-25-11_20.00sec_-5.00C_LIGHT_0838.fits
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.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_Cyg-03-Q2b1x1_022658_TTUQ2b1x1_12955_x3T21hfc/wcs_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839.fits
Preparing the HTML report for the field Cyg-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out224268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out233768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out102581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out224275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73582.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
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: 9s
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Considering the candidate 224268_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 224268_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:03:34.31 +46:49:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.364 2085735800843373312 300.89323305332 +46.82515684214 13.0483 12.4763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 224273_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 224273_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:11:24.44 +46:53:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224275_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 224275_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 224277_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 224277_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:01:00.94 +45:50:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224285_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 224285_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:03:53.75 +41:49:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224287_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 224287_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:09:10.43 +44:53:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225581_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 225581_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 225822_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 225822_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225939_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 225939_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227056_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 227056_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 229664_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 229664_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:49:00.51 +46:08:21.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 230307_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 230307_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 19:59:14.71 +45:45:14.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 231426_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 231426_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:31:30.06 +49:11:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232689_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 232689_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:45:07.86 +45:44:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233009_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 233009_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:11:09.42 +47:07:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233144_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 233144_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:15:20.87 +47:40:37.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 233768_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 233768_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:20:18.94 +49:25:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 3.564 2084737306850122112 305.07778529880 +49.42363426347 11.8299 10.6306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 233885_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 233885_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 19:59:12.30 +48:43:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234010_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 234010_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234217_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 234217_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:19:45.01 +47:52:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235654_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 235654_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:22:14.83 +45:46:39.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236172_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 236172_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:30:57.79 +49:13:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 4.077 2180034006851686912 307.74127249144 +49.22292145860 12.7012 11.8586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236230_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 236230_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:21:49.62 +48:59:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236383_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 236383_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:06:00.53 +45:00:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.051 2082211140223031552 301.50108804685 +45.00238473432 12.7019 12.2502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236617_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 236617_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:17:38.45 +42:43:09.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236662_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 236662_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 238336_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 238336_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:38:01.78 +47:58:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 238346_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 238346_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:30:03.04 +45:53:59.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 238616_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 238616_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 239024_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 239024_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:05:41.58 +47:45:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239791_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 239791_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:12:12.39 +46:19:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239819_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 239819_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:03:45.59 +47:42:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77882_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 77882_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:44:58.92 +47:08:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120386_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 120386_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:41:25.30 +45:16:50.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 78384_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 78384_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:15:28.61 +47:42:47.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 135769_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 135769_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:45:58.62 +44:28:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101382_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 101382_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:13:38.28 +46:44:27.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 45277_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 45277_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:44:17.29 +48:34:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20414_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 20414_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 211242_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 211242_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:22:59.25 +50:03:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97925_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 97925_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:02:27.55 +46:43:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68384_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 68384_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:38:03.57 +47:40:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173015_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 173015_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 54267_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 54267_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:05:44.28 +48:32:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107251_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 107251_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 53609_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 53609_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 112147_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 112147_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:18:00.93 +46:05:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93587_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 93587_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:46:43.89 +46:28:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135527_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 135527_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:40:12.35 +44:37:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51738_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 51738_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 127946_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 127946_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:30:18.16 +45:11:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133307_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 133307_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:22:08.38 +45:00:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103637_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 103637_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:41:10.80 +46:08:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92833_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 92833_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:19:08.30 +46:53:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127540_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 127540_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 28088_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 28088_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 30523_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 30523_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:20:24.98 +49:42:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108148_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 108148_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:48:01.63 +45:47:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21642_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 21642_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 20278_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 20278_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 137436_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 137436_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:42:08.70 +44:25:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188739_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 188739_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:46:36.31 +42:44:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88936_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 88936_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:33:37.94 +46:58:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107666_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 107666_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:37:34.12 +46:01:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33492_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 33492_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:34:06.01 +49:21:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114334_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 114334_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:40:16.42 +45:42:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140140_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 140140_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 25122_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 25122_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:01:27.71 +50:02:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125183_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 125183_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:49:03.25 +44:59:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133705_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 133705_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:40:15.10 +44:41:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127446_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 127446_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:48:34.03 +44:52:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22169_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 22169_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 192640_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 192640_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:35:03.31 +43:10:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116838_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 116838_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 136933_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 136933_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:43:40.30 +44:28:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73582_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 73582_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 67328_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 67328_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 194425_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 194425_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:43:09.08 +43:13:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172273_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 172273_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:38:26.18 +41:52:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91746_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 91746_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:46:48.94 +46:34:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131947_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 131947_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:35:12.62 +44:53:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111173_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 111173_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:47:54.09 +45:41:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93945_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 93945_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:36:43.91 +46:38:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179862_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 179862_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:34:01.34 +42:25:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128362_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 128362_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:44:51.19 +44:55:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79703_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 79703_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:44:48.64 +47:03:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147611_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 147611_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:45:10.91 +43:40:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59754_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 59754_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:43:20.75 +47:57:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186438_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 186438_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:28:06.49 +42:55:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174004_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 174004_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:07:19.68 +42:16:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189987_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 189987_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:17:59.53 +43:17:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171021_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 171021_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 140134_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 140134_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:13:40.62 +44:37:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113035_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 113035_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 102581_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 102581_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 24348_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 24348_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 50416_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 50416_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 181251_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 181251_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:45:13.70 +42:20:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67304_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 67304_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:33:00.98 +47:46:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120068_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 120068_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:22:05.53 +45:47:43.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116588_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 116588_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:29:53.41 +45:45:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124593_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 124593_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:16:00.77 +45:34:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 95638_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 95638_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:33:54.83 +46:41:38.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 27614_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
Preparing report for the candidate 27614_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
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Considering the candidate 98315_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 98315_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:13:18.37 +46:48:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170595_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 170595_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:05:31.56 +42:04:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44610_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 44610_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:30:03.48 +48:57:03.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189601_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 189601_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:13:42.98 +43:22:45.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 40240_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 40240_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:31:18.73 +49:13:09.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 36727_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 36727_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:27:02.44 +49:23:00.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 182112_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 182112_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:17:29.09 +42:43:20.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 115993_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 115993_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:47:20.67 +45:34:47.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196446_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 196446_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:40:02.92 +43:27:31.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103876_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 103876_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:48:56.22 +46:06:51.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62825_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 62825_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
**** FOUND 20:47:49.22 +47:49:54.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170698_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839
The candidate 170698_fd_Cyg-03-Q2b1x1_2026-04-14_02-26-01_20.00sec_-4.90C_LIGHT_0839 did not pass the final checks
