This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz
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 10.1452* 04 19 08.99 +40 45 42.2 11.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GL Per,2461140.6452,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GL Per 20260410.1452 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 03 39.54 +33 43 34.5 13.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J060.9167+33.7274,2461140.6452,13.00,0.05,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 J060.9167+33.7274 20260410.1452 13.00CV 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 10.1452* 04 17 50.91 +41 17 06.9 14.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6452,13.98,0.05,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
VARIABLE_NAME 20260410.1452 13.98CV 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 10.1452* 04 00 16.87 +39 18 15.5 12.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J040016.66+391816.3,2461140.6452,12.80,0.05,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
ASASSN-V J040016.66+391816.3 20260410.1452 12.80CV 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
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 10.1452* 04 43 16.09 +41 43 15.2 12.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044316.36+414317.4,2461140.6452,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J044316.36+414317.4 20260410.1452 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 23 09.46 +41 43 03.2 11.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042309.53+414305.5,2461140.6452,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042309.53+414305.5 20260410.1452 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 16 07.87 +41 39 31.3 10.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0647 Per,2461140.6452,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0647 Per 20260410.1452 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 12 57.81 +39 14 16.9 12.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4207171,2461140.6452,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4207171 20260410.1452 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 03 59 26.99 +38 54 53.6 12.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J035926.82+385453.9,2461140.6452,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J035926.82+385453.9 20260410.1452 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 42 28.40 +41 32 30.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0442287+413231,2461140.6452,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0442287+413231 20260410.1452 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 01 03.64 +34 18 11.0 13.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6452,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1452 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 02 00.95 +33 49 17.8 12.9 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6452,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1452 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 04 00.50 +35 01 16.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6452,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1452 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 10 03.48 +39 04 48.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IRAS 04066+3857,2461140.6452,13.34,0.05,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
IRAS 04066+3857 20260410.1452 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 10.1452* 04 12 55.20 +38 24 54.8 12.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041255.15+382455.1,2461140.6452,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041255.15+382455.1 20260410.1452 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 05 18.11 +41 20 58.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0405176+412058,2461140.6452,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0405176+412058 20260410.1452 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1452* 04 36 04.05 +34 10 43.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0436047+341041,2461140.6452,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0436047+341041 20260410.1452 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461140.64551830 10.04.2026 03:29:22.781 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 13703
Objects passed selection criteria: 13667
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: 11806.8
Average stars matched: 11465.5 (97.1097 %)
Memory usage VmPeak: 119980 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:31:43 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 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: 2461140.64551830 10.04.2026 03:29:22.781 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 150
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: 35 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): 111286
Objects passed selection criteria: 111033
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 88915.8
Average stars matched: 85532.5 (96.195 %)
Memory usage VmPeak: 1886352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:33:42 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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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: 2461140.64486993
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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits exists and is non-empty
Saving wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits'
wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits exists and is non-empty
Saving wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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 04:21:42.834 +37:58:42.50
Angular distance between the image centers 0.0317 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 04:21:42.675 +37:59:08.11
Angular distance between the image centers 0.0275 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 04:21:42.834 +37:58:42.50
Second-epoch second image center 04:21:42.675 +37:59:08.11
Angular distance between the image centers 0.00713 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.iG13bX0K0k
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.wfT6Xg9j0N
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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits &> /tmp/tmp.xuMzygLpFE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits &> /tmp/tmp.96ORw7kwdQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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 4 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
3.0 pix fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
2.9 pix fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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
14.5 mag. fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
14.5 mag. fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.9 (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.iG13bX0K0k (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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...
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...
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
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"
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.wfT6Xg9j0N (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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...
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...
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
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"
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.xuMzygLpFE (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=934, passed=10710
Got 10710 stars (including 9767 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 10710 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 10454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
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 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 10456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 10456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Excluding outliers - 948 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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.96ORw7kwdQ (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=988, passed=10657
Got 10657 stars (including 9662 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 10657 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 10399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
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 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 943 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits'
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out06850.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03543_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 03543_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:00:21.19 +42:02:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08921_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 08921_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:48:28.53 +39:16:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08101_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 08101_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:37:53.84 +39:56:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06850_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 06850_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
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 ####
04:19:08.99 +40:45:42.2
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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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 04:21:42.834 +37:58:42.50
Angular distance between the image centers 0.0317 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 04:21:42.675 +37:59:08.11
Angular distance between the image centers 0.0275 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 04:21:42.834 +37:58:42.50
Second-epoch second image center 04:21:42.675 +37:59:08.11
Angular distance between the image centers 0.00713 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.ImCqQpzyZS
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.SuMlqRuJXT
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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits &> /tmp/tmp.A454tPyOMz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits &> /tmp/tmp.AXS5lZQUZg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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 79 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
2.8 pix fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
2.8 pix fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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
14.6 mag. fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
14.6 mag. fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ImCqQpzyZS (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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...
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...
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
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"
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.SuMlqRuJXT (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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...
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...
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
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"
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.A454tPyOMz (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=6682, passed=63828
Got 63828 stars (including 57058 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 63828 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 62095 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 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 62095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 62095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AXS5lZQUZg (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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.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_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=6557, passed=63511
Got 63511 stars (including 56879 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 63511 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 61581 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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 61580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 61580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
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_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits -region wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/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_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/wcs_fd_Per-05-Q2b1x1_2026-04-09_22-28-26_20.00sec_-4.90C_LIGHT_0002.fits
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-05-Q2b1x1_223009_TTUQ2b1x1_4576_tfisHadz/wcs_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003.fits
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out166904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out106984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82279.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166904_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166904_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:41:36.55 +34:07:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 3.607 173524890737264128 070.40311181350 +34.12337578021 14.0391 12.9864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166908_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166908_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:28:38.11 +42:07:22.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166913_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166913_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:47:48.08 +38:46:44.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166916_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166916_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:06:53.88 +39:40:56.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166922_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166922_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:56:46.97 +41:57:32.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)
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Considering the candidate 166924_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166924_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:00:47.79 +34:01:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.801 218603222506063104 060.20071818283 +34.03057591113 13.1154 12.3532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166927_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166927_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:05:08.23 +36:47:46.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 166935_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166935_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:25:37.52 +40:23:02.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 166936_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 166936_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 166943_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 166943_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:51:56.03 +42:03:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167197_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167197_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:00:35.67 +34:00:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 3.542 218602329152874880 060.14784274177 +34.01209343581 11.1213 9.9784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167216_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167216_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:35:11.65 +39:19:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167281_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167281_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:12:12.47 +39:26:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167429_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167429_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:51:41.57 +42:03:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167498_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167498_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:24:32.96 +34:09:19.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167602_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167602_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:24:35.91 +34:06:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167647_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167647_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:17:52.06 +42:00:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167655_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167655_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:12:48.65 +40:37:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167696_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167696_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:24:35.37 +34:07:11.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167777_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167777_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:55:23.67 +40:35:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167845_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167845_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:55:16.87 +38:45:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.987 199108877047308544 073.82051331208 +38.76318519265 13.2511 12.0377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167858_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167858_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:53:41.73 +38:47:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167905_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167905_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:51:34.81 +35:48:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167930_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167930_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:55:23.55 +40:34:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.656 200102015223159680 073.85011534336 +40.58057161653 13.6334 12.6091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167986_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 167986_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:13:17.67 +33:49:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168004_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168004_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:55:08.56 +39:55:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.635 200015566122061184 073.78582338050 +39.92271568273 13.7652 13.3062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168012_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168012_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:45:31.38 +35:43:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168082_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168082_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:25:38.27 +40:26:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168091_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168091_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:29:54.56 +39:50:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168096_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168096_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:35:31.58 +37:29:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168098_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168098_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:40:37.89 +39:21:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168117_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168117_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:48:13.07 +39:57:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.702 200200799471664768 072.05471287333 +39.96375091823 13.9998 13.0864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168146_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168146_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:02:08.30 +33:38:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.380 170541198434116736 060.53364065556 +33.64415366917 13.0621 11.9534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168157_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168157_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:34:03.63 +41:18:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 5.121 203892542904647168 068.51404384996 +41.31247332461 13.8410 12.8897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168185_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168185_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:43:29.17 +34:32:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168223_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168223_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:31:59.24 +36:43:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168336_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168336_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:23:11.39 +35:29:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168371_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 168371_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 168376_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168376_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:50:31.81 +41:29:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168385_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168385_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:44:56.95 +35:36:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168421_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 168421_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 88105_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 88105_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:08:15.27 +37:43:34.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84307_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 84307_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:08:37.29 +38:02:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66200_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 66200_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:48:28.53 +39:16:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71422_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 71422_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 80666_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 80666_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:07:53.58 +38:31:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93060_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 93060_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:16:01.26 +37:20:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26080_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 26080_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 31477_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 31477_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 48567_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 48567_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:19:09.02 +40:45:41.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 118111_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 118111_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:15:40.63 +35:32:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31520_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 31520_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 119373_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 119373_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:21:30.83 +35:35:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72465_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 72465_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 58905_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 58905_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:37:53.81 +39:56:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28143_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 28143_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:21:25.50 +41:52:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76363_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 76363_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 118886_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 118886_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:27:10.46 +35:29:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29987_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 29987_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 86548_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 86548_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:21:52.18 +37:56:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64442_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 64442_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:10:26.38 +39:49:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127385_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 127385_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 141889_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 141889_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 91744_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 91744_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 60877_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 60877_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:23:32.56 +40:01:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.147 227610657982197376 065.88627348198 +40.02640705102 12.4276 10.7854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25134_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 25134_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:00:21.21 +42:02:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76697_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 76697_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:13:39.10 +38:55:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157769_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 157769_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:11:07.99 +40:08:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92682_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 92682_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:17:06.07 +37:22:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112595_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 112595_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 74785_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 74785_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 82279_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 82279_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 28944_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 28944_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:27:32.35 +41:47:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38349_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 38349_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 77091_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 77091_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:15:00.36 +38:52:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106984_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
Preparing report for the candidate 106984_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
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Considering the candidate 85442_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 85442_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:05:31.51 +38:05:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69838_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 69838_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
**** FOUND 04:16:24.24 +39:25:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32067_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003
The candidate 32067_fd_Per-05-Q2b1x1_2026-04-09_22-29-22_20.00sec_-4.90C_LIGHT_0003 did not pass the final checks
