This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 12.14 01:40:22.31 +09:44:42.8
142.42874 -51.26465 galactic Psc Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.124 Alkeste -0 1 1 12.2 -0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:40:22.31 +09:44:42.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:40:22.31 +09:44:42.8: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 12.14CV 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
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 14.91 01:55:39.00 +06:24:04.3
150.13247 -53.04562 galactic Psc Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.580 Selene -1 -1 1 15.2 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:55:39.00 +06:24:04.3: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:55:39.00 +06:24:04.3: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,14.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 14.91CV 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
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 13.07 01:14:58.94 +03:48:44.6
134.23907 -58.54152 galactic Psc Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.58 Concordia -0 -0 0 13.2 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:14:58.94 +03:48:44.6: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:14:58.94 +03:48:44.6: 15.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 13.07CV 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
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 13.30 01:45:39.35 +03:23:41.1
148.22016 -56.79123 galactic Psc Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.329 Svea -0 -0 1 13.4 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:45:39.35 +03:23:41.1: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:45:39.35 +03:23:41.1: 16.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 13.30CV 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
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 13.62 01:50:44.85 +09:33:32.6
146.35639 -50.59552 galactic Psc Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.167 Urda -0 0 0 13.8 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:50:44.85 +09:33:32.6: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:50:44.85 +09:33:32.6: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 14.07 01:20:58.69 +02:03:53.5
137.79630 -59.95161 galactic Cet Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.522 Helga -0 -1 1 14.0 0 -0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:20:58.69 +02:03:53.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:20:58.69 +02:03:53.5: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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 09 19.3811* 01 20 58.69 +02 03 53.5 14.1 U Cet 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,2461302.8811,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 14.07CV 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
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 14.14 01:33:06.22 +03:20:03.8
142.80027 -57.92109 galactic Psc Second-epoch detections are separated by 1.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1235 Schorria 0 -0 0 14.6 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:33:06.22 +03:20:03.8: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:33:06.22 +03:20:03.8: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 14.14CV 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
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 14.22 02:03:50.46 +10:28:26.4
150.38789 -48.49998 galactic Psc Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.401 Ottilia -1 -0 1 14.6 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:03:50.46 +10:28:26.4: 15.82 +/- 0.34 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:03:50.46 +10:28:26.4: 15.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.82 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 14.22CV 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
Mean magnitude and position on the discovery images:
2026 09 19.3811 2461302.8811 14.39 01:37:06.77 +06:10:07.1
142.95871 -54.91729 galactic Psc Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.885 Ulrike -1 1 1 14.5 -0 -0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:37:06.77 +06:10:07.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:37:06.77 +06:10:07.1: 16.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8811,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260919.3811 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
First image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Last image: 2461302.88137954 19.09.2026 09:09:01.192 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 6718
Objects passed selection criteria: 6711
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 6311.5
Average stars matched: 6149.5 (97.4333 %)
Memory usage VmPeak: 232740 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Sep 19 04:10:44 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
First image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Last image: 2461302.88137954 19.09.2026 09:09:01.192 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 49
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 11 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 35804
Objects passed selection criteria: 35705
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 34146.2
Average stars matched: 32779 (95.9959 %)
Memory usage VmPeak: 256708 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Sep 19 04:11:35 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/TTUQ1b1x1/TTUQ1_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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat to cache
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461302.88082146
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_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (1st reference image)
verification OK: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:52.061 +05:59:58.49 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits (1st new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:30.988 +06:02:15.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:52.061 +05:59:58.49
Second-epoch image center 01:42:30.988 +06:02:15.02
Angular distance between the image centers 0.0952 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits (2nd new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:32.912 +06:01:42.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:52.061 +05:59:58.49
Second-epoch image center 01:42:32.912 +06:01:42.28
Angular distance between the image centers 0.0844 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 01:42:30.988 +06:02:15.02
Second-epoch second image center 01:42:32.912 +06:01:42.28
Angular distance between the image centers 0.01209 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.mJqq5DIaz3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits &> /tmp/tmp.ucMC9aLdis
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits &> /tmp/tmp.0jNgnaHJnc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits &> /tmp/tmp.2vEaYw89wE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
The reference image (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits) and catalog (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat) found
'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat' -> 'wcsmag.cat'
Read 6596 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7251 to 33.6950 deg, Dec +0.7082 to +11.2853 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 17.7251 to 33.6950 deg, Dec 0.7082 to 11.2853 deg
Loaded 4460 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): 3591 out of 3785 total matches.
Matched with Tycho-2 3785 out of 6596 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.907900
a=0.000000 b=1.000000 c=22.907900
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6596 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7251 to 33.6950 deg, Dec +0.7082 to +11.2853 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 17.7251 to 33.6950 deg, Dec 0.7082 to 11.2853 deg
Loaded 4460 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): 3591 out of 3785 total matches.
Matched with Tycho-2 3785 out of 6596 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (aperture=5.9)
Read 6518 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7253 to 33.6950 deg, Dec +0.6952 to +11.2758 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 17.7253 to 33.6950 deg, Dec 0.6952 to 11.2758 deg
Loaded 4461 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): 3569 out of 3774 total matches.
Matched with Tycho-2 3774 out of 6518 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits (aperture=5.9)
____ 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: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
2.0 pix Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
2.2 pix fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
2.1 pix fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Limiting magnitude estimates:
15.4 mag. Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
15.4 mag. Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
15.3 mag. fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
15.3 mag. fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.mJqq5DIaz3 (6) ############
Parsing command line arguments...
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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=487, bad_region=0, passed=6596
Got 6596 stars (including 6101 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
util/solve_plate_with_UCAC5 got 6596 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 4867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4867 stars left (next iteration limit 5353)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits N_match=4867 sigma_overall_arcsec=0.269 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.257 sigma_q3_arcsec=0.237 sigma_q4_arcsec=0.240 n_q1=1229 n_q2=1222 n_q3=1222 n_q4=1194 worst_quadrant_to_overall_ratio=1.283
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ucMC9aLdis (6) ############
Parsing command line arguments...
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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, bad_region=0, passed=6518
Got 6518 stars (including 6013 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat
util/solve_plate_with_UCAC5 got 6518 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 6518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4867 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits N_match=4867 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.262 sigma_q3_arcsec=0.273 sigma_q4_arcsec=0.250 n_q1=1217 n_q2=1224 n_q3=1230 n_q4=1196 worst_quadrant_to_overall_ratio=1.332
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0jNgnaHJnc (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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=487, bad_region=0, passed=6173
Got 6173 stars (including 5682 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat
util/solve_plate_with_UCAC5 got 6173 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 6173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 6173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 6173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4863 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4863 robust_rms=10.747 arcsec worst_quadrant_rms=11.989 arcsec
SIP_REFIT: SIP order 3 trial: matched=4863 robust_rms=0.491 arcsec worst_quadrant_rms=0.579 arcsec
SIP_REFIT: SIP order 5 trial: matched=4863 robust_rms=0.325 arcsec worst_quadrant_rms=0.402 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4863 robust_rms_before=1.079 arcsec robust_rms_before_corrected=0.321 arcsec robust_rms_after=0.325 arcsec worst_quadrant_rms_before=0.391 worst_quadrant_rms_after=0.402
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.391 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits N_match=4863 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.310 sigma_q4_arcsec=0.306 n_q1=1267 n_q2=1195 n_q3=1217 n_q4=1184 worst_quadrant_to_overall_ratio=1.173
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits -region wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2vEaYw89wE (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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=490, bad_region=0, passed=6117
Got 6117 stars (including 5622 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat
util/solve_plate_with_UCAC5 got 6117 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 6117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 6117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 6117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4859 stars left (next iteration limit 5344)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4859 robust_rms=10.816 arcsec worst_quadrant_rms=11.848 arcsec
SIP_REFIT: SIP order 3 trial: matched=4859 robust_rms=0.510 arcsec worst_quadrant_rms=0.603 arcsec
SIP_REFIT: SIP order 5 trial: matched=4859 robust_rms=0.348 arcsec worst_quadrant_rms=0.421 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4859 robust_rms_before=1.076 arcsec robust_rms_before_corrected=0.344 arcsec robust_rms_after=0.348 arcsec worst_quadrant_rms_before=0.403 worst_quadrant_rms_after=0.421
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.403 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits N_match=4859 sigma_overall_arcsec=0.347 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.332 n_q1=1255 n_q2=1185 n_q3=1223 n_q4=1196 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits -region wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits to local_wcs_cache/
'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits' -> 'local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits'
Saving the final (post-refit) wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits to local_wcs_cache/
'wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits' -> 'local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits'
Saving the final (post-refit) wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits'
Saving the final (post-refit) wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits sigma_overall=0.269 worst_q_ratio=1.283
ref2=Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits sigma_overall=0.286 worst_q_ratio=1.332
new1=fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits sigma_overall=0.327 worst_q_ratio=1.173
new2=fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits sigma_overall=0.347 worst_q_ratio=1.118
reference average sigma_overall=0.2775 worst_q_ratio=1.3075
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_astrometric_residuals.png (4867 matched stars from wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_astrometric_residuals.png (4867 matched stars from wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418_astrometric_residuals.png (4863 matched stars from wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419_astrometric_residuals.png (4859 matched stars from wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits'
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits'
Preparing the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:40:22.31 +09:44:42.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:24.54 +09:25:18.4: 12.32 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:00:11.59 +01:16:13.4: 12.44 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:50:24.99 +10:19:55.6: 12.38 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:11.59 +01:16:13.4: 12.39 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:00:24.54 +09:25:18.4: 12.34 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:50:24.99 +10:19:55.6: 12.38 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:40:22.31 +09:44:42.8: 15.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 02:00:24.54 +09:25:18.4: ref_mag=12.33 +/- 0.01 new_mean_mag=12.2894 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:00:11.59 +01:16:13.4: ref_mag=12.41 +/- 0.01 new_mean_mag=12.3087 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:50:24.99 +10:19:55.6: ref_mag=12.38 +/- 0.01 new_mean_mag=12.3218 delta=0.06 (need > 0.90)
Adding exclusion_list_local.txt__out20437.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 20437_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 20437_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20458_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 20458_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20460_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 20460_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20464_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 20464_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:40:22.31 +09:44:42.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat to cache
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Creating symlink local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Checking 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_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (1st reference image)
verification OK: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:52.061 +05:59:58.49 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits (1st new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:30.988 +06:02:15.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:52.061 +05:59:58.49
Second-epoch image center 01:42:30.988 +06:02:15.02
Angular distance between the image centers 0.0952 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits (2nd new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:32.912 +06:01:42.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:52.061 +05:59:58.49
Second-epoch image center 01:42:32.912 +06:01:42.28
Angular distance between the image centers 0.0844 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 01:42:30.988 +06:02:15.02
Second-epoch second image center 01:42:32.912 +06:01:42.28
Angular distance between the image centers 0.01209 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.QLZ4p5p32a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits &> /tmp/tmp.tYJoiC4i4J
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits &> /tmp/tmp.XaVZ2tUdGJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits &> /tmp/tmp.uElrlXD2da
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
The reference image (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits) and catalog (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat) found
'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat' -> 'wcsmag.cat'
Read 34861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7251 to 33.6950 deg, Dec +0.7049 to +11.2866 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 17.7251 to 33.6950 deg, Dec 0.7049 to 11.2866 deg
Loaded 4462 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): 3472 out of 3869 total matches.
Matched with Tycho-2 3869 out of 34861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.813000
a=0.000000 b=1.000000 c=22.813000
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7251 to 33.6950 deg, Dec +0.7049 to +11.2866 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 17.7251 to 33.6950 deg, Dec 0.7049 to 11.2866 deg
Loaded 4462 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): 3472 out of 3869 total matches.
Matched with Tycho-2 3869 out of 34861 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (aperture=4.8)
Read 35044 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7253 to 33.7129 deg, Dec +0.6952 to +11.2770 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 17.7253 to 33.7129 deg, Dec 0.6952 to 11.2770 deg
Loaded 4464 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): 3471 out of 3871 total matches.
Matched with Tycho-2 3871 out of 35044 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
1.9 pix Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
2.0 pix fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
1.9 pix fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Limiting magnitude estimates:
15.5 mag. Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
15.5 mag. Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
15.5 mag. fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
15.5 mag. fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QLZ4p5p32a (6) ############
Parsing command line arguments...
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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1454, bad_region=1, passed=34850
Got 34850 stars (including 33348 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat
util/solve_plate_with_UCAC5 got 34850 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 34850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 34850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 34850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4874 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits N_match=4874 sigma_overall_arcsec=0.259 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.257 sigma_q3_arcsec=0.231 sigma_q4_arcsec=0.233 n_q1=1228 n_q2=1207 n_q3=1228 n_q4=1211 worst_quadrant_to_overall_ratio=1.251
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tYJoiC4i4J (6) ############
Parsing command line arguments...
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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1474, bad_region=5, passed=35030
Got 35030 stars (including 33485 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat
util/solve_plate_with_UCAC5 got 35030 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 35030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 35030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 35030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4875 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits N_match=4875 sigma_overall_arcsec=0.284 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.263 sigma_q3_arcsec=0.268 sigma_q4_arcsec=0.242 n_q1=1228 n_q2=1205 n_q3=1241 n_q4=1201 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.XaVZ2tUdGJ (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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1378, bad_region=37, passed=33754
Got 33754 stars (including 32287 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat
util/solve_plate_with_UCAC5 got 33754 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 33754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 33754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 33754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4869 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4869 robust_rms=10.564 arcsec worst_quadrant_rms=11.941 arcsec
SIP_REFIT: SIP order 3 trial: matched=4869 robust_rms=0.486 arcsec worst_quadrant_rms=0.577 arcsec
SIP_REFIT: SIP order 5 trial: matched=4869 robust_rms=0.313 arcsec worst_quadrant_rms=0.384 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4869 robust_rms_before=1.065 arcsec robust_rms_before_corrected=0.307 arcsec robust_rms_after=0.313 arcsec worst_quadrant_rms_before=0.381 worst_quadrant_rms_after=0.384
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.381 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits N_match=4869 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.297 n_q1=1285 n_q2=1204 n_q3=1215 n_q4=1165 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits -region wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.uElrlXD2da (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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1395, bad_region=34, passed=33879
Got 33879 stars (including 32389 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat
util/solve_plate_with_UCAC5 got 33879 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 33879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 33879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 33879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4870 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4870 robust_rms=10.511 arcsec worst_quadrant_rms=11.709 arcsec
SIP_REFIT: SIP order 3 trial: matched=4870 robust_rms=0.508 arcsec worst_quadrant_rms=0.595 arcsec
SIP_REFIT: SIP order 5 trial: matched=4870 robust_rms=0.338 arcsec worst_quadrant_rms=0.421 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4870 robust_rms_before=1.065 arcsec robust_rms_before_corrected=0.334 arcsec robust_rms_after=0.338 arcsec worst_quadrant_rms_before=0.408 worst_quadrant_rms_after=0.421
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.408 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits N_match=4870 sigma_overall_arcsec=0.338 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.378 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.337 n_q1=1281 n_q2=1199 n_q3=1212 n_q4=1178 worst_quadrant_to_overall_ratio=1.121
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits -region wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-08-12_20.00sec_-0.00C_LIGHTs_0418.fits
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.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_2026-09-19_CI_Psc-06-Q1b1x1_040944_TTUQ1b1x1_2896449_Cx2V2rjp/wcs_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419.fits
Preparing the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:11:00.12 +10:13:17.5: 14.48 +/- 0.11 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:56:10.05 +10:47:47.6: 13.87 +/- 0.05 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:03:17.10 +01:57:12.4: 14.28 +/- 0.09 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:27:57.63 +05:37:42.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:02:15.69 +10:06:31.3: 14.64 +/- 0.11 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:05:36.97 +01:45:37.3: 14.75 +/- 0.14 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:45:30.98 +09:29:00.9: 14.44 +/- 0.08 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:55:39.00 +06:24:04.3: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:33:15.82 +05:53:08.8: 14.58 +/- 0.09 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:21:29.99 +03:46:27.7: 12.88 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:02:15.69 +10:06:31.3: 14.53 +/- 0.10 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:27:57.63 +05:37:42.7: 13.67 +/- 0.04 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:11:00.12 +10:13:17.5: 14.56 +/- 0.11 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:45:30.98 +09:29:00.9: 14.36 +/- 0.07 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:55:39.00 +06:24:04.3: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:05:36.97 +01:45:37.3: 14.81 +/- 0.15 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:56:10.05 +10:47:47.6: 13.88 +/- 0.05 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:03:17.10 +01:57:12.4: 14.11 +/- 0.07 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:33:15.82 +05:53:08.8: 14.71 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry reference-image weighted average: 14.58 +/- 0.07
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Forced photometry reference-image weighted average: 14.52 +/- 0.08
Forced photometry filter REJECTED candidate at 01:27:57.63 +05:37:42.7: ref_mag=13.68 +/- 0.03 new_mean_mag=14.0517 delta=-0.37 (need > 0.90)
Forced photometry reference-image weighted average: 14.39 +/- 0.05
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Forced photometry filter REJECTED candidate at 02:11:00.12 +10:13:17.5: ref_mag=14.52 +/- 0.08 new_mean_mag=14.5239 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:02:15.69 +10:06:31.3: ref_mag=14.58 +/- 0.07 new_mean_mag=14.5113 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:05:36.97 +01:45:37.3: ref_mag=14.78 +/- 0.10 new_mean_mag=14.5388 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.64 +/- 0.06
Forced photometry reference-image weighted average: 14.18 +/- 0.05
Forced photometry filter REJECTED candidate at 01:45:30.98 +09:29:00.9: ref_mag=14.39 +/- 0.05 new_mean_mag=14.5669 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:56:10.05 +10:47:47.6: ref_mag=13.87 +/- 0.04 new_mean_mag=14.3308 delta=-0.46 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:33:15.82 +05:53:08.8: ref_mag=14.64 +/- 0.06 new_mean_mag=14.9207 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:03:17.10 +01:57:12.4: ref_mag=14.18 +/- 0.05 new_mean_mag=14.3010 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:21:29.99 +03:46:27.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter REJECTED candidate at 01:21:29.99 +03:46:27.7: ref_mag=12.86 +/- 0.01 new_mean_mag=12.9146 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:50:44.85 +09:33:32.6: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:20:58.69 +02:03:53.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:39:29.51 +02:43:30.9: 11.45 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:14:58.94 +03:48:44.6: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:23:49.85 +06:29:03.7: 13.86 +/- 0.06 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:45:39.35 +03:23:41.1: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:10:40.11 +10:10:40.4: 13.52 +/- 0.05 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:33:06.22 +03:20:03.8: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:03:50.46 +10:28:26.4: 15.82 +/- 0.34 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:50:44.85 +09:33:32.6: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:20:58.69 +02:03:53.5: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:14:58.94 +03:48:44.6: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:45:39.35 +03:23:41.1: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:10:40.11 +10:10:40.4: 13.51 +/- 0.05 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:39:29.51 +02:43:30.9: 11.46 +/- 0.01 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:23:49.85 +06:29:03.7: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry reference-image weighted average: 11.46 +/- 0.00
Forced photometry filter REJECTED candidate at 02:10:40.11 +10:10:40.4: ref_mag=13.51 +/- 0.03 new_mean_mag=13.8169 delta=-0.31 (need > 0.90)
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Forced photometry filter REJECTED candidate at 01:39:29.51 +02:43:30.9: ref_mag=11.46 +/- 0.00 new_mean_mag=11.8941 delta=-0.44 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:23:49.85 +06:29:03.7: ref_mag=13.80 +/- 0.04 new_mean_mag=13.8429 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:33:06.22 +03:20:03.8: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:03:50.46 +10:28:26.4: 15.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.82 +/- 0.34
Forced photometry filter KEPT candidate at 02:03:50.46 +10:28:26.4: ref_mag=15.82 +/- 0.34 new_mean_mag=14.2077 delta=1.61 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:18:24.02 +04:55:45.9: 14.93 +/- 0.15 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:58:03.19 +03:22:11.5: 15.05 +/- 0.16 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:37:06.77 +06:10:07.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:18:24.02 +04:55:45.9: 15.04 +/- 0.17 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:58:03.19 +03:22:11.5: 15.05 +/- 0.15 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:37:06.77 +06:10:07.1: 16.19 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.98 +/- 0.11
Forced photometry reference-image weighted average: 15.05 +/- 0.11
Forced photometry filter REJECTED candidate at 01:18:24.02 +04:55:45.9: ref_mag=14.98 +/- 0.11 new_mean_mag=14.5564 delta=0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:58:03.19 +03:22:11.5: ref_mag=15.05 +/- 0.11 new_mean_mag=14.4604 delta=0.59 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:14:22.54 +09:26:58.1: 14.96 +/- 0.17 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:09.52 +03:31:37.0: 14.95 +/- 0.15 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:14:22.54 +09:26:58.1: 14.93 +/- 0.17 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:09.52 +03:31:37.0: 14.91 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.12
Forced photometry reference-image weighted average: 14.93 +/- 0.10
Forced photometry filter REJECTED candidate at 02:14:22.54 +09:26:58.1: ref_mag=14.94 +/- 0.12 new_mean_mag=14.8022 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:25:09.52 +03:31:37.0: ref_mag=14.93 +/- 0.10 new_mean_mag=14.7482 delta=0.18 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:23:50.91 +03:43:46.6: 14.91 +/- 0.14 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:15:00.01 +02:53:02.7: 14.66 +/- 0.13 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:23:50.91 +03:43:46.6: 15.09 +/- 0.16 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:15:00.01 +02:53:02.7: 14.88 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.10
Forced photometry filter REJECTED candidate at 01:23:50.91 +03:43:46.6: ref_mag=14.98 +/- 0.10 new_mean_mag=14.8078 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 14.74 +/- 0.10
Forced photometry filter REJECTED candidate at 01:15:00.01 +02:53:02.7: ref_mag=14.74 +/- 0.10 new_mean_mag=14.8023 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:13:06.77 +07:46:29.0: 15.42 +/- 0.25 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 02:09:55.34 +09:50:46.5: 15.36 +/- 0.23 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:13:06.77 +07:46:29.0: 15.18 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.16
Forced photometry filter REJECTED candidate at 02:13:06.77 +07:46:29.0: ref_mag=15.27 +/- 0.16 new_mean_mag=14.8589 delta=0.41 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 02:09:55.34 +09:50:46.5: 15.44 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.17
Forced photometry filter REJECTED candidate at 02:09:55.34 +09:50:46.5: ref_mag=15.40 +/- 0.17 new_mean_mag=14.9326 delta=0.46 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:20:20.40 +08:45:47.6: 15.14 +/- 0.18 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:22:35.30 +04:45:57.7: 14.70 +/- 0.13 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:22:35.30 +04:45:57.7: 15.04 +/- 0.18 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:20:20.40 +08:45:47.6: 15.09 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.10
Forced photometry reference-image weighted average: 15.11 +/- 0.12
Forced photometry filter REJECTED candidate at 01:22:35.30 +04:45:57.7: ref_mag=14.81 +/- 0.10 new_mean_mag=14.6916 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:20:20.40 +08:45:47.6: ref_mag=15.11 +/- 0.12 new_mean_mag=14.9026 delta=0.21 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:15:47.24 +09:27:33.4: 15.23 +/- 0.21 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:15:43.85 +02:21:51.5: 14.95 +/- 0.17 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:15:43.85 +02:21:51.5: 15.22 +/- 0.22 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:15:47.24 +09:27:33.4: 15.03 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.13
Forced photometry reference-image weighted average: 15.11 +/- 0.13
Forced photometry filter REJECTED candidate at 01:15:43.85 +02:21:51.5: ref_mag=15.05 +/- 0.13 new_mean_mag=14.8035 delta=0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:15:47.24 +09:27:33.4: ref_mag=15.11 +/- 0.13 new_mean_mag=14.9120 delta=0.20 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:12:01.15 +01:28:56.3: 15.41 +/- 0.28 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:20:45.93 +01:47:10.8: 14.95 +/- 0.16 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:20:45.93 +01:47:10.8: 15.17 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.12
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:12:01.15 +01:28:56.3: 14.94 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 01:20:45.93 +01:47:10.8: ref_mag=15.04 +/- 0.12 new_mean_mag=14.8706 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 15.08 +/- 0.15
Forced photometry filter REJECTED candidate at 01:12:01.15 +01:28:56.3: ref_mag=15.08 +/- 0.15 new_mean_mag=14.6694 delta=0.41 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:15:17.27 +09:46:49.1: 14.92 +/- 0.15 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:15:27.84 +03:02:01.1: 14.83 +/- 0.15 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:15:17.27 +09:46:49.1: 15.11 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.12
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:15:27.84 +03:02:01.1: 14.97 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 01:15:17.27 +09:46:49.1: ref_mag=15.00 +/- 0.12 new_mean_mag=14.9548 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.89 +/- 0.11
Forced photometry filter REJECTED candidate at 01:15:27.84 +03:02:01.1: ref_mag=14.89 +/- 0.11 new_mean_mag=14.6978 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:25:15.58 +10:18:50.1: 15.16 +/- 0.17 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:14:48.21 +04:11:20.9: 14.64 +/- 0.12 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:18:30.11 +08:36:04.6: 15.06 +/- 0.16 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:25:15.58 +10:18:50.1: 15.17 +/- 0.17 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:14:48.21 +04:11:20.9: 14.72 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.12
Forced photometry reference-image weighted average: 14.68 +/- 0.09
Forced photometry filter REJECTED candidate at 01:25:15.58 +10:18:50.1: ref_mag=15.17 +/- 0.12 new_mean_mag=14.9684 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:14:48.21 +04:11:20.9: ref_mag=14.68 +/- 0.09 new_mean_mag=14.6577 delta=0.02 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:18:30.11 +08:36:04.6: 15.52 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.14
Forced photometry filter REJECTED candidate at 01:18:30.11 +08:36:04.6: ref_mag=15.20 +/- 0.14 new_mean_mag=14.9741 delta=0.22 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:17:07.30 +03:57:11.5: 14.82 +/- 0.14 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits at 01:22:56.62 +04:54:47.2: 15.18 +/- 0.17 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:17:07.30 +03:57:11.5: 15.12 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.11
Forced photometry filter REJECTED candidate at 01:17:07.30 +03:57:11.5: ref_mag=14.93 +/- 0.11 new_mean_mag=14.7619 delta=0.17 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits at 01:22:56.62 +04:54:47.2: 15.50 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.14
Forced photometry filter REJECTED candidate at 01:22:56.62 +04:54:47.2: ref_mag=15.29 +/- 0.14 new_mean_mag=15.0014 delta=0.29 (need > 0.90)
Adding exclusion_list_local.txt__out52380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53233.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 52379_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52379_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52380_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 52380_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 52385_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52385_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52387_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52387_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52388_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52388_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
**** FOUND 01:38:56.81 +10:39:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52389_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52389_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52390_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52390_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52391_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52391_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52392_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52392_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52393_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52393_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52397_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52397_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52399_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52399_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52550_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52550_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
**** FOUND 01:40:22.31 +09:44:42.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52704_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 52704_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 52764_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 52764_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 52827_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 52827_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 52870_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52870_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 52906_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 52906_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53063_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 53063_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 53085_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 53085_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 53093_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 53093_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 53213_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53213_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53233_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
Preparing report for the candidate 53233_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
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Considering the candidate 53240_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53240_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53297_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53297_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53343_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53343_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53362_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53362_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53366_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53366_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53411_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53411_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53416_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53416_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53420_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53420_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53421_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53421_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53433_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53433_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53442_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53442_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53445_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53445_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53458_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53458_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53461_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53461_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53462_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53462_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53465_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53465_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53478_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53478_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53491_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53491_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53504_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53504_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 53517_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 53517_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
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Considering the candidate 25189_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 25189_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
**** FOUND 01:40:17.98 +01:39:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50793_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419
The candidate 50793_fd_Psc-06-Q1b1x1_2026-09-19_04-09-01_20.00sec_-0.00C_LIGHTs_0419 did not pass the final checks
