This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1
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!
TCP 2026 04 06.1008* 04 03 07.11 +35 11 17.9 13.9 U Per 9 0
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 219056805412912256,2461136.6008,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 219056805412912256 20260406.1008 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 03 52 54.95 +33 51 40.2 13.4 U Per 9 0
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 218727261161944192,2461136.6008,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 218727261161944192 20260406.1008 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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!
TCP 2026 04 06.1008* 03 57 54.77 +36 17 08.3 13.1 U Per 9 0
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 J059.4739+36.2905,2461136.6008,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J059.4739+36.2905 20260406.1008 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 04 38 24.61 +37 21 43.3 14.2 U Per 9 0
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 J069.6076+37.3610,2461136.6008,14.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J069.6076+37.3610 20260406.1008 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 04 37 53.85 +39 56 15.9 12.0 U Per 9 0
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
HL Per,2461136.6008,11.97,0.05,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
HL Per 20260406.1008 11.97CV 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!
TCP 2026 04 06.1008* 04 21 52.22 +37 56 41.6 13.9 U Per 9 0
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
NSVS J0421526+375642,2461136.6008,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0421526+375642 20260406.1008 13.88CV 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!
TCP 2026 04 06.1008* 04 05 31.47 +38 05 12.9 12.7 U Per 9 0
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 J040531.19+380511.8,2461136.6008,12.66,0.05,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
ASASSN-V J040531.19+380511.8 20260406.1008 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!
TCP 2026 04 06.1008* 04 15 00.31 +38 52 38.3 13.3 U Per 9 0
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 J041500.30+385239.7,2461136.6008,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041500.30+385239.7 20260406.1008 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 04 21 30.80 +35 35 40.3 13.4 U Per 9 0
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
CSS_J042130.8+353538,2461136.6008,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J042130.8+353538 20260406.1008 13.41CV 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!
TCP 2026 04 06.1008* 04 18 07.10 +36 22 29.2 13.3 U Per 9 0
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
NSVS J0418072+362229,2461136.6008,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0418072+362229 20260406.1008 13.34CV 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!
TCP 2026 04 06.1008* 04 10 26.41 +39 49 38.0 13.2 U Per 9 0
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
ZTF J041026.22+394939.3,2461136.6008,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J041026.22+394939.3 20260406.1008 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 03 54 36.81 +38 06 01.9 12.5 U Per 9 0
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
GSC 02864-01273,2461136.6008,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 02864-01273 20260406.1008 12.51CV 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!
TCP 2026 04 06.1008* 04 13 38.99 +38 55 09.9 13.1 U Per 9 0
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
NSVS J0413388+385513,2461136.6008,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0413388+385513 20260406.1008 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 04 17 06.16 +37 22 20.4 13.2 U Per 9 0
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 J041706.01+372219.1,2461136.6008,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041706.01+372219.1 20260406.1008 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 03 53 21.39 +38 51 15.2 11.6 U Per 9 0
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 J035320.89+385115.3,2461136.6008,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J035320.89+385115.3 20260406.1008 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1008* 03 54 35.43 +38 04 28.1 13.8 U Per 9 0
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
2MASS J03543503+3804273,2461136.6008,13.80,0.05,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
2MASS J03543503+3804273 20260406.1008 13.80CV 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: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
First image: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Last image: 2461136.60112538 06.04.2026 02:25:27.233 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15190
Objects passed selection criteria: 15167
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 13840.2
Average stars matched: 13453.2 (97.2038 %)
Memory usage VmPeak: 120676 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 21:29:24 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: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
First image: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Last image: 2461136.60112538 06.04.2026 02:25:27.233 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 169
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 41 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): 119177
Objects passed selection criteria: 118940
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 103436
Average stars matched: 99579.2 (96.2718 %)
Memory usage VmPeak: 1897044 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 21:31:10 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/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
SExtractor catalog cache: saved Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.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: 2461136.60043637
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_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits exists and is non-empty
Saving wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits to local_wcs_cache/
'wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits exists and is non-empty
Saving wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits to local_wcs_cache/
'wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> 'local_wcs_cache/wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits'
wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:49.829 +37:59:58.29
Angular distance between the image centers 0.0014 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:52.748 +37:59:21.79
Angular distance between the image centers 0.0153 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:21:49.829 +37:59:58.29
Second-epoch second image center 04:21:52.748 +37:59:21.79
Angular distance between the image centers 0.01395 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/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits &> /tmp/tmp.xun6GHZrfK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits &> /tmp/tmp.5LrXAdQWHy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits &> /tmp/tmp.sC3w7MVw1V
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits &> /tmp/tmp.KcRclYS95j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
Found non-empty wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
The reference image (wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits) and catalog (wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat) found
'wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat' -> 'wcsmag.cat'
Read 18830 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9680 to 76.3320 deg, Dec +32.2038 to +43.3213 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 54.9680 to 76.3320 deg, Dec 32.2038 to 43.3213 deg
Loaded 9186 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): 6363 out of 7115 total matches.
Matched with Tycho-2 7115 out of 18830 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.972881
a=0.000000 b=1.000000 c=22.972881
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
2.0 pix Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
2.6 pix fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
2.6 pix fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Limiting magnitude estimates:
15.5 mag. Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
15.5 mag. Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
14.9 mag. fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
14.9 mag. fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xun6GHZrfK (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/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> 'wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1807, passed=18830
Got 18830 stars (including 16990 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 18830 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits -region wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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.5LrXAdQWHy (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/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> 'wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1869, passed=18776
Got 18776 stars (including 16879 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 18776 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 18312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 18314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 18314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits -region wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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.sC3w7MVw1V (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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1321, passed=13591
Got 13591 stars (including 12253 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 13591 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 952 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: 951 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 13127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 13128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 13128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.KcRclYS95j (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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1296, passed=13643
Got 13643 stars (including 12335 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 13643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 952 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: 951 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 13261 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 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 13260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 13260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 950 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits'
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21422.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 21114_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 21114_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:43:53.86 +40:43:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.730 202935967786660096 070.97467397801 +40.72108329002 12.0897 11.6616 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21357_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 21357_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:30:34.79 +38:56:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.605 179590965105796352 067.64517139589 +38.94666568595 11.7917 10.9076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21390_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 21390_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:47:39.65 +39:42:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.092 199821090002070528 071.91596097387 +39.71610486244 11.2357 9.9878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21401_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 21401_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:56:53.98 +40:05:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.667 200030306449627136 074.22515877032 +40.09944940163 12.2973 11.7517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21409_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 21409_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:44:07.79 +37:26:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.540 175331152119355904 071.03298735768 +37.43564193102 12.2243 11.5054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21422_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 21422_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:44:00.98 +39:36:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.053 202804851027290624 071.00446293960 +39.61036304951 11.8683 10.7813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03543_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 03543_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:00:21.31 +42:02:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06850_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 06850_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:19:09.02 +40:45:42.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
SExtractor catalog cache: saved Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Creating symlink local_wcs_cache/wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.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_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits exists and is non-empty
wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:49.829 +37:59:58.29
Angular distance between the image centers 0.0014 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:52.748 +37:59:21.79
Angular distance between the image centers 0.0153 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:21:49.829 +37:59:58.29
Second-epoch second image center 04:21:52.748 +37:59:21.79
Angular distance between the image centers 0.01395 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/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits &> /tmp/tmp.1vfU9LH8RU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits &> /tmp/tmp.c5ZpxTamSR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits &> /tmp/tmp.QHMWnKstrp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits &> /tmp/tmp.eGdRu4gcrk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
Found non-empty wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
The reference image (wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits) and catalog (wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat) found
'wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat' -> 'wcsmag.cat'
Read 145138 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9680 to 76.3546 deg, Dec +32.1479 to +43.3235 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 54.9680 to 76.3546 deg, Dec 32.1479 to 43.3235 deg
Loaded 9259 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): 5279 out of 7192 total matches.
Matched with Tycho-2 7192 out of 145138 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.821281
a=0.000000 b=1.000000 c=22.821281
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 94 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
1.8 pix Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
2.5 pix fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
2.5 pix fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Limiting magnitude estimates:
15.6 mag. Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
15.6 mag. Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
15.0 mag. fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
15.0 mag. fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.1vfU9LH8RU (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/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> 'wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=15711, passed=145118
Got 145118 stars (including 129130 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 145118 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 141865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 141863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 141862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits -region wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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.c5ZpxTamSR (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/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> 'wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=15921, passed=145731
Got 145731 stars (including 129503 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 145731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 142089 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 142089 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 142089 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits -region wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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.QHMWnKstrp (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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=10108, passed=85801
Got 85801 stars (including 75579 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 85801 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 923 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: 952 matched stars entering correct_measured_positions(), 82839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 82838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 82839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 951 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eGdRu4gcrk (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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=10264, passed=85767
Got 85767 stars (including 75375 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 85767 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 949 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: 948 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 82879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
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: 947 matched stars entering correct_measured_positions(), 82879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 82880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 947 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_Per-05-Q2b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-24-27_20.00sec_-4.90C_LIGHT_0018.fits
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q2b1x1_212611_TTUQ2b1x1_22090_ZJeXAfB1/wcs_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019.fits
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out157901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out167509.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out119373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92682.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 9s
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Considering the candidate 167452_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167452_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:47:44.27 +39:06:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.650 199719110299061248 071.93421367997 +39.10444494039 14.9762 14.1896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167455_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167455_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:10:05.60 +38:19:33.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 167456_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167456_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:47:40.58 +36:28:22.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)
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Considering the candidate 167459_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167459_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:49:25.70 +35:31:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.239 174124850424892160 072.35706381585 +35.52696341256 14.3112 13.3212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167465_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167465_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 167483_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 167483_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 167488_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167488_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:52:40.91 +34:19:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.112 218793094420498816 058.17213407638 +34.32309849883 13.1545 12.6551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167505_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167505_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:52:18.59 +34:51:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.659 219592989130133632 058.07839482251 +34.86355693046 12.6467 12.1280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167506_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167506_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:52:54.04 +34:12:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.401 218788627654544128 058.22490841498 +34.21311822214 12.8136 12.1613 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 167507_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167507_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:59:34.07 +35:58:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.038 219384872194486784 059.89201524449 +35.97249044517 13.6253 13.1175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167508_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167508_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:15:37.15 +37:15:55.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
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Considering the candidate 167509_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167509_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:58:09.83 +38:09:16.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 167510_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167510_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:52:37.33 +34:27:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.750 218829550102856576 058.15612954633 +34.45657553353 12.9072 12.2287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167514_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167514_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:59:15.74 +33:50:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 5.267 218579651725603840 059.81608909506 +33.84229046970 13.0250 12.3603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167515_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167515_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:51:55.14 +34:53:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167521_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 167521_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 167543_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167543_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:01:35.47 +36:30:52.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 167544_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167544_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:52:53.06 +34:13:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.572 218788829513937408 058.22110225991 +34.23259133159 12.4879 11.7981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167552_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167552_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:22.83 +34:22:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.588 218813572824513920 058.34548207596 +34.36954470632 12.2148 11.6005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167553_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167553_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:23.72 +33:59:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.396 218734163171617920 058.34783320559 +33.98374271411 12.4270 11.7520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167554_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167554_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:00.84 +34:19:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.683 218792613384143488 058.25179138431 +34.33256972211 12.1901 11.5717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167555_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 167555_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167559_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167559_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:00.13 +34:13:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.036 218788657715246208 058.24942199223 +34.22453428450 12.2240 11.6457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167564_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167564_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:51:56.05 +42:03:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167569_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167569_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:28:51.03 +41:45:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167571_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167571_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:52:47.61 +34:38:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.983 218836009733597184 058.19688344527 +34.64183198044 11.8862 11.3696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167572_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167572_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:08:37.18 +39:59:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167574_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167574_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:50:30.13 +39:16:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 2.263 223944890511091840 057.62476537377 +39.26650993301 11.7197 11.1956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167576_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167576_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:12:12.37 +39:26:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.588 226249569962168320 063.05173661736 +39.44747992668 11.0835 9.5891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167577_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167577_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:45.40 +33:40:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 5.889 218708736965220992 058.44077850114 +33.66857514110 11.7152 11.1462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167917_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 167917_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:35:11.64 +39:19:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168090_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168090_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:58:46.61 +35:47:50.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 168092_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168092_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:51:41.61 +42:03:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168279_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168279_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:17:52.23 +42:00:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168362_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168362_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:15:31.29 +33:49:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168524_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168524_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:53:41.78 +38:47:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168648_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168648_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:29:54.39 +39:50:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168658_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168658_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:56:27.56 +41:15:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.087 201639128183008640 074.11445936633 +41.26388192897 14.0464 13.4979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168683_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168683_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:55:59.61 +40:10:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168696_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168696_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:15:53.09 +41:37:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.944 228729930753431936 063.97061308947 +41.61964012058 14.5874 13.7512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168709_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168709_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:13:17.88 +33:49:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168763_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168763_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:20:14.37 +34:32:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168778_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168778_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:45:31.35 +35:43:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168782_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168782_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:40:37.96 +39:21:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168799_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168799_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:46:18.03 +39:14:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.090 199738660990018560 071.57480260701 +39.24560742954 14.2742 13.5907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168809_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168809_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:23:11.42 +35:29:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168818_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168818_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:19:56.96 +41:05:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168830_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168830_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:54:49.44 +40:39:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 3.850 200114865765313792 073.70705637839 +40.65504173633 14.1448 13.5494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168841_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168841_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 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 168872_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168872_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:35:31.54 +37:29:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.365 178463660747111552 068.88224295822 +37.49368150163 13.6119 12.6455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168915_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168915_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:31:59.36 +36:43:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.525 178051859282479104 067.99753215832 +36.71609460503 13.9591 12.9564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168962_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168962_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:08:08.72 +37:44:38.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 168975_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168975_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:56:01.27 +40:10:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168998_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 168998_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:49:35.12 +39:13:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169060_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169060_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:39:24.96 +42:11:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169065_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169065_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:44:56.87 +35:36:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 3.478 174286753511957760 071.23774967941 +35.60708466206 14.1117 13.3623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169080_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169080_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:23:12.34 +35:29:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169160_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 169160_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 169207_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169207_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:23:59.48 +41:56:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.700 228327818739227136 065.99845055406 +41.94102678352 14.0373 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169209_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169209_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:43:29.16 +34:32:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 3.072 173654293807134080 070.87221839848 +34.53857981443 14.0910 12.3219 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169254_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169254_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:56:01.66 +40:00:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169259_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169259_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:55:52.43 +41:47:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.282 201875317025022976 073.96830961488 +41.79078275660 14.5715 14.2036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169260_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169260_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:50:31.76 +41:29:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.791 203381686612203264 072.63335834111 +41.49427360949 13.4707 11.4675 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169304_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169304_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:29:15.16 +39:20:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169305_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169305_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:08:14.38 +36:36:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169466_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169466_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:27:42.78 +41:41:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.780 228189452072145280 066.92727867244 +41.69370973636 14.4938 13.8678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169493_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169493_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:31:39.13 +37:40:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169526_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169526_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:55:27.22 +38:47:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 0.614 199109392443380096 073.86363540551 +38.79652399175 14.7381 13.9216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169701_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169701_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:46:38.30 +40:39:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.546 203246515400935680 071.65971007940 +40.66070077436 14.5179 13.7039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169754_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 169754_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:28:00.02 +38:31:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.998 179199989940138368 067.00076806516 +38.52114460703 14.6560 13.3254 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58905_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 58905_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 118886_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 118886_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:27:10.52 +35:29:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86548_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 86548_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 85442_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 85442_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 77091_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 77091_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 48567_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 48567_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:19:09.05 +40:45:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80666_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 80666_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:07:53.55 +38:31:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119373_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 119373_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 129623_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 129623_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 64442_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 64442_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 84734_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 84734_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 93060_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 93060_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:16:01.38 +37:20:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112619_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 112619_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:43.53 +35:00:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76697_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 76697_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 92682_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 92682_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 25134_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 25134_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:00:21.36 +42:02:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28944_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 28944_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:27:32.39 +41:47:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157901_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 157901_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:11:08.00 +40:08:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.511 227063376068008192 062.78278483879 +40.14917774138 12.0847 10.3159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 76362_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
Preparing report for the candidate 76362_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
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Considering the candidate 69838_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 69838_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:16:24.22 +39:25:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32067_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 32067_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:13:47.33 +41:42:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66200_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 66200_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
**** FOUND 04:48:28.48 +39:16:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156124_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019
The candidate 156124_fd_Per-05-Q2b1x1_2026-04-05_21-25-27_20.00sec_-4.90C_LIGHT_0019 did not pass the final checks
