This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2045032945549053056,2461135.8845,12.67,0.05,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 2045032945549053056 20260405.3845 12.67CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.1361+31.0639,2461135.8845,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.1361+31.0639 20260405.3845 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.7754+28.7734,2461135.8845,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.7754+28.7734 20260405.3845 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2032465974354931968,2461135.8845,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2032465974354931968 20260405.3845 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2032636536065313280,2461135.8845,12.53,0.05,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
Gaia DR3 2032636536065313280 20260405.3845 12.53CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.6459+32.5159,2461135.8845,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.6459+32.5159 20260405.3845 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194321.36+313118.5,2461135.8845,12.40,0.05,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 J194321.36+313118.5 20260405.3845 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193719.50+305226.2,2461135.8845,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193719.50+305226.2 20260405.3845 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1863726463109169664,2461135.8845,12.24,0.05,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 1863726463109169664 20260405.3845 12.24CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193111.81+323346.5,2461135.8845,12.04,0.05,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
ASASSN-V J193111.81+323346.5 20260405.3845 12.04CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2046993752753683200,2461135.8845,11.96,0.05,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 2046993752753683200 20260405.3845 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01319,2461135.8845,12.03,0.05,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
HAT 199-01319 20260405.3845 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.1568+31.4986,2461135.8845,12.50,0.05,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 J294.1568+31.4986 20260405.3845 12.50CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J306.9220+30.1703,2461135.8845,12.71,0.05,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 J306.9220+30.1703 20260405.3845 12.71CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2024488880063184128,2461135.8845,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2024488880063184128 20260405.3845 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.1947+29.3247,2461135.8845,12.72,0.05,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
ATO J298.1947+29.3247 20260405.3845 12.72CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.2177+30.4488,2461135.8845,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.2177+30.4488 20260405.3845 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461135.88479966 05.04.2026 09:13:56.691 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 24877
Objects passed selection criteria: 24771
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 17308.2
Average stars matched: 16773 (96.9075 %)
Memory usage VmPeak: 130140 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 04:18:26 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: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
First image: 2461098.99239403 27.02.2026 11:48:52.844 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Last image: 2461135.88479966 05.04.2026 09:13:56.691 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 186
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 71 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): 230092
Objects passed selection criteria: 229439
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 165624
Average stars matched: 159038 (96.024 %)
Memory usage VmPeak: 2146196 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 04:25:58 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.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: 2461135.88422595
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits'
wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits exists and is non-empty
Saving wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits to local_wcs_cache/
'wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.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 20:00:00.965 +30:00:24.17
Second-epoch image center 20:00:15.419 +30:01:10.16
Angular distance between the image centers 0.0537 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 20:00:00.965 +30:00:24.17
Second-epoch image center 20:00:12.765 +30:01:05.11
Angular distance between the image centers 0.0441 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 20:00:15.419 +30:01:10.16
Second-epoch second image center 20:00:12.765 +30:01:05.11
Angular distance between the image centers 0.00968 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.h21R2vK6rg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.ITqpaSTaxc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits &> /tmp/tmp.HXssVHM3V1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits &> /tmp/tmp.FkbmEkn5v4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat' -> 'wcsmag.cat'
Read 30878 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.2644 to 309.4609 deg, Dec +24.2020 to +35.3348 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 290.2644 to 309.4609 deg, Dec 24.2020 to 35.3348 deg
Loaded 30795 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): 6699 out of 7455 total matches.
Matched with Tycho-2 7455 out of 30878 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854269
a=0.000000 b=1.000000 c=22.854269
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
2.0 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
2.9 pix fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
2.9 pix fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Limiting magnitude estimates:
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
14.9 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
13.2 mag. fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
13.3 mag. fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.h21R2vK6rg (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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3756, passed=30878
Got 30878 stars (including 27089 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 30878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 571 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 641 matched stars entering correct_measured_positions(), 569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.90"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 631 matched stars entering correct_measured_positions(), 19509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.54"
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 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 701 matched stars entering correct_measured_positions(), 19538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.51"
WARNING: Accuracy estimation diagnostic: 698 matched stars entering correct_measured_positions(), 21385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.18"
Excluding outliers - 698 stars left (next iteration limit 694)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.ITqpaSTaxc (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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3771, passed=30931
Got 30931 stars (including 27121 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 30931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 571 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 610 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 541 matched stars entering correct_measured_positions(), 474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.80"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 533 matched stars entering correct_measured_positions(), 15522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.95"
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 571 to 628 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 585 matched stars entering correct_measured_positions(), 15534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.91"
WARNING: Accuracy estimation diagnostic: 583 matched stars entering correct_measured_positions(), 16703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.33"
Excluding outliers - 583 stars left (next iteration limit 586)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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.HXssVHM3V1 (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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=737, passed=8706
Got 8706 stars (including 7967 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 8706 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 8382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 8379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 8380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FkbmEkn5v4 (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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=749, passed=9017
Got 9017 stars (including 8258 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 9017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 8525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 8525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 8522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits'
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits'
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cyg-08-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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat to cache
SExtractor catalog cache: saved Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits exists and is non-empty
wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.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 20:00:00.965 +30:00:24.17
Second-epoch image center 20:00:15.419 +30:01:10.16
Angular distance between the image centers 0.0537 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 20:00:00.965 +30:00:24.17
Second-epoch image center 20:00:12.765 +30:01:05.11
Angular distance between the image centers 0.0441 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 20:00:15.419 +30:01:10.16
Second-epoch second image center 20:00:12.765 +30:01:05.11
Angular distance between the image centers 0.00968 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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.xsEWfKDEPu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.709M5oWE20
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits &> /tmp/tmp.CTGfc6LTvz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits &> /tmp/tmp.ztOmLlUsbz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
Found non-empty wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits and wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
The reference image (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits) and catalog (wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat) found
'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat' -> 'wcsmag.cat'
Read 281578 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 290.2219 to 309.4679 deg, Dec +24.1963 to +35.3349 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 290.2219 to 309.4679 deg, Dec 24.1963 to 35.3349 deg
Loaded 30877 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): 5684 out of 8842 total matches.
Matched with Tycho-2 8842 out of 281578 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.629178
a=0.000000 b=1.000000 c=22.629178
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 85 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
1.9 pix Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
2.4 pix fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
2.4 pix fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Limiting magnitude estimates:
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
15.0 mag. Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
13.6 mag. fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
13.6 mag. fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.0 (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.xsEWfKDEPu (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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=51531, passed=281520
Got 281520 stars (including 229582 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 281520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 692 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 642 matched stars entering correct_measured_positions(), 589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.01"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 635 matched stars entering correct_measured_positions(), 211069 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 754 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 715 matched stars entering correct_measured_positions(), 211109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.27"
WARNING: Accuracy estimation diagnostic: 713 matched stars entering correct_measured_positions(), 228657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.36"
Excluding outliers - 713 stars left (next iteration limit 698)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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.709M5oWE20 (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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits' -> 'wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=51082, passed=280646
Got 280646 stars (including 229187 good ones) from the SExtractor catalog wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 280646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 570 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 584 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 520 matched stars entering correct_measured_positions(), 457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.56"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 517 matched stars entering correct_measured_positions(), 153986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.22"
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 570 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 627 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 567 matched stars entering correct_measured_positions(), 154010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.22"
WARNING: Accuracy estimation diagnostic: 567 matched stars entering correct_measured_positions(), 174936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 567 stars left (next iteration limit 568)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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.CTGfc6LTvz (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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=9076, passed=85954
Got 85954 stars (including 76785 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 85954 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 83472 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 83469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 83468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ztOmLlUsbz (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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Checking if the catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
WCS catalog name: wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=9427, passed=87195
Got 87195 stars (including 77680 good ones) from the SExtractor catalog wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 87195 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 84364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 84362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 84362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits -region wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits
Saving fully-calibrated image wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.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_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_Cyg-08-Q2b1x1_2026-02-27_05-49-53_20.00sec_-15.00C_LIGHT_0040.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-07_20.00sec_-4.90C_LIGHT_0171.fits
Saving fully-calibrated image wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cyg-08-Q2b1x1_041548_TTUQ2b1x1_27257_hBit41Dg/wcs_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172.fits
Preparing the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out132242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317030.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 28s
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: 10s
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Considering the candidate 316805_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316805_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:52:13.10 +26:52:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.075 2027155676755633152 298.05430722394 +26.87492887085 13.3194 12.2929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316815_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316815_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:03:27.40 +27:58:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.238 2028954683934676096 300.86373090753 +27.98116509449 13.7944 13.0301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316827_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316827_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:25:25.46 +29:44:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.355 1860539910922857088 306.35601008706 +29.74274019988 13.1190 12.3566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316834_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316834_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:50:05.14 +31:56:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.295 2033792638215545344 297.52171606145 +31.94722086409 13.0591 12.6386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316838_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316838_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:05:23.63 +27:29:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.730 1836725171948359040 301.34841012241 +27.48405184538 13.3050 12.4873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316849_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316849_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316852_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316852_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:02:49.51 +26:49:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.693 1835176960819264896 300.70589738658 +26.82850660505 13.5285 12.8584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316860_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316860_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:57:01.59 +26:26:59.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 316869_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316869_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:31:07.67 +28:41:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 4.553 2026289669596200960 292.78336822033 +28.69068114502 12.4868 12.0589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316873_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316873_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:51:32.12 +28:38:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.876 2028639467733414528 297.88376200927 +28.64279714394 12.5082 11.4043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316878_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316878_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:40:29.78 +33:20:30.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)
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Considering the candidate 316895_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316895_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:57:46.41 +28:29:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.473 2027743090854652032 299.44291018514 +28.48530004484 12.9564 12.4572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316897_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316897_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:48:29.75 +32:49:02.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)
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Considering the candidate 316900_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316900_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316903_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316903_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:48:00.70 +30:53:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 2.096 2032176253037333760 297.00224105990 +30.88863603826 12.4370 11.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316906_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316906_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:46:00.65 +33:59:29.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 316907_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316907_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:25:09.33 +30:23:39.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 316923_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316923_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:27:54.11 +30:59:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.307 1861838571595809024 306.97506955181 +30.99206036351 12.7210 11.8344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316924_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316924_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316925_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316925_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316926_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316926_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:34:14.86 +27:28:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316929_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316929_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316931_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316931_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:34:59.05 +29:50:17.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)
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Considering the candidate 316934_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316934_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316938_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316938_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:43:51.28 +33:53:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.281 2047047590130241792 295.96258217888 +33.88741375001 12.6065 11.8558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316940_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316940_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316942_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316942_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:38:14.01 +33:11:50.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
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Considering the candidate 316955_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316955_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:29:09.82 +30:59:37.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)
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Considering the candidate 316960_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316960_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316962_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316962_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 316963_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316963_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316967_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316967_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:30:02.97 +27:03:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.765 2024924046138405760 292.51134276638 +27.06101996325 12.4815 11.6128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316970_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316970_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:34:31.52 +28:28:54.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)
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Considering the candidate 316971_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316971_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:46:54.82 +33:05:15.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
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Considering the candidate 316977_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 316977_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 316983_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316983_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:24:04.11 +30:22:26.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)
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Considering the candidate 316985_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316985_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:20:20.07 +27:42:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316988_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316988_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:23:58.27 +28:54:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316989_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316989_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:55:16.62 +33:59:51.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)
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Considering the candidate 316990_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316990_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:25:38.01 +29:20:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.992 1860494762225134336 306.40835359175 +29.33797511154 12.4771 12.0253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316991_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316991_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:30:31.02 +27:21:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.269 2025308428529772800 292.62934882141 +27.36248694520 12.3021 11.2471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 316994_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 316994_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:55:44.77 +32:19:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317019_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317019_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:28:24.20 +30:56:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.630 1861834276628347520 307.10103604531 +30.93615970120 11.3543 10.1536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317021_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 317021_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 317023_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317023_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:26:36.18 +29:12:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317029_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317029_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:29:47.06 +31:08:06.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)
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Considering the candidate 317030_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 317030_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 317034_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317034_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:23:41.06 +29:19:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.768 1860502561886399616 305.92114436602 +29.32206759985 12.1974 11.3788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317035_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317035_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:27:12.96 +30:55:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.007 1861743498197428096 306.80413531489 +30.92774558737 12.3467 11.8104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317038_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317038_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:28:11.23 +31:51:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.756 1861947595042749952 307.04719609680 +31.85879524889 12.1952 11.8768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317041_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317041_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:55:35.22 +32:58:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317042_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317042_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:40:58.13 +31:04:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.967 2032939417194293248 295.24092683797 +31.06768117774 12.7201 12.3040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317044_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317044_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:32:29.27 +26:59:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.107 2025234310226859264 293.12225412499 +26.99673053332 11.7712 10.7399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317046_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317046_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:32:00.49 +28:20:07.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)
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Considering the candidate 317047_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317047_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:24:38.83 +28:54:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317052_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317052_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 317053_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317053_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:24:08.87 +29:47:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.177 1861270738246309248 306.03702967703 +29.79342893246 11.5232 10.6770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317054_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317054_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:29:29.14 +31:09:24.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)
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Considering the candidate 317055_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317055_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:27:56.54 +31:12:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317062_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317062_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:34:03.22 +31:46:04.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)
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Considering the candidate 317194_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317194_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:27:57.17 +30:08:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317230_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317230_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:49:51.28 +27:06:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317250_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317250_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:44:46.66 +29:14:26.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 317270_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317270_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:25:38.58 +30:21:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317326_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317326_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:51:15.66 +26:35:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317343_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317343_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:28:03.93 +34:10:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.997 2056117740733847296 307.01643462955 +34.17844962958 10.4763 9.7652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317345_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317345_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:50:56.59 +26:49:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317356_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317356_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:53:22.78 +26:28:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317379_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317379_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:24:43.54 +29:18:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317416_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317416_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:27:50.28 +31:00:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.401 1861839323197003008 306.95955254748 +31.01136229794 12.6626 11.7513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 317535_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 317535_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:04:06.57 +25:48:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293756_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 293756_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:30:40.59 +26:51:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195333_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 195333_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:25:13.87 +32:11:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.923 1862196703152178176 306.30752330591 +32.19676640319 11.6062 11.2649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186452_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 186452_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 44695_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 44695_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:00:42.84 +26:59:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110658_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 110658_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:52:10.46 +29:21:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293367_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 293367_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:55:21.95 +26:47:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35023_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 35023_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 19:32:08.30 +26:06:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132242_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 132242_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 295891_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 295891_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
**** FOUND 20:27:55.77 +30:59:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26604_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 26604_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 295627_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 295627_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 295449_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
Preparing report for the candidate 295449_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
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Considering the candidate 236091_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 236091_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 188289_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172
The candidate 188289_fd_Cyg-08-Q2b1x1_2026-04-05_04-13-56_20.00sec_-5.00C_LIGHT_0172 did not pass the final checks
