This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh
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 10 21.2887 2461334.7887 10.63 01:55:37.09 +09:38:08.5
148.05862 -50.07877 galactic Psc Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -0 -0 0 10.7 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:55:37.09 +09:38:08.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:55:37.09 +09:38:08.5: 15.78 +/- 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,2461334.7887,10.63,0.05,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 20261021.2887 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.2887 2461334.7887 12.70 01:30:15.44 +14:04:39.9
137.00125 -47.73073 galactic Psc Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.295 Theresia -0 -0 0 12.9 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:15.44 +14:04:39.9: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:30:15.44 +14:04:39.9: 15.97 +/- 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,2461334.7887,12.70,0.05,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 20261021.2887 12.70CV 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 10 21.2887 2461334.7887 12.97 01:28:44.33 +11:22:31.0
137.37769 -50.44730 galactic Psc Second-epoch detections are separated by 0.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.147 Protogeneia -0 -0 0 12.9 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:44.33 +11:22:31.0: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:44.33 +11:22:31.0: 15.89 +/- 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,2461334.7887,12.97,0.05,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 20261021.2887 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.2887 2461334.7887 13.30 02:16:36.77 +13:36:24.5
152.49275 -44.32135 galactic Ari Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.257 Silesia -0 -0 0 13.6 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:16:36.77 +13:36:24.5: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:16:36.77 +13:36:24.5: 15.83 +/- 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 10 21.2887* 02 16 36.77 +13 36 24.5 13.3 U Ari 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,2461334.7887,13.30,0.05,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 20261021.2887 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 10 21.2887 2461334.7887 13.52 01:20:45.92 +16:44:51.0
132.98195 -45.55118 galactic Psc Second-epoch detections are separated by 1.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1572 Posnania -1 0 1 13.6 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:20:45.92 +16:44:51.0: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:20:45.92 +16:44:51.0: 15.76 +/- 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,2461334.7887,13.52,0.05,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 20261021.2887 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.2887 2461334.7887 13.64 01:42:53.26 +09:15:44.1
143.61398 -51.53158 galactic Psc Second-epoch detections are separated by 0.9" and 6.8 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 -1 1 13.9 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:53.26 +09:15:44.1: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:42:53.26 +09:15:44.1: 15.98 +/- 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,2461334.7887,13.64,0.05,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 20261021.2887 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.2887 2461334.7887 13.95 02:14:13.89 +10:03:38.8
154.09536 -47.73855 galactic Cet Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.99 Dike 0 0 0 13.8 0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:14:13.89 +10:03:38.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:14:13.89 +10:03:38.8: 15.83 +/- 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 10 21.2887* 02 14 13.89 +10 03 38.8 13.9 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,2461334.7887,13.95,0.05,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 20261021.2887 13.95CV 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 10 21.2887 2461334.7887 14.22 01:52:08.65 +13:27:09.5
144.77918 -46.82778 galactic Ari Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1146 Biarmia 0 -1 1 14.2 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:08.65 +13:27:09.5: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:52:08.65 +13:27:09.5: 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!
TCP 2026 10 21.2887* 01 52 08.65 +13 27 09.5 14.2 U Ari 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,2461334.7887,14.22,0.05,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 20261021.2887 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 10 21.2887 2461334.7887 14.28 01:28:33.26 +11:19:30.9
137.32623 -50.50625 galactic Psc Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2675 Tolkien -1 -1 1 14.1 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:33.26 +11:19:30.9: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:33.26 +11:19:30.9: 15.89 +/- 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,2461334.7887,14.28,0.05,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 20261021.2887 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.2887 2461334.7887 14.49 01:40:35.32 +10:17:00.2
142.25282 -50.73530 galactic Psc Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2976 Lautaro -0 -0 0 14.7 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:35.32 +10:17:00.2: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:40:35.32 +10:17:00.2: 15.98 +/- 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,2461334.7887,14.49,0.05,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 20261021.2887 14.49CV 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 10 21.2887 2461334.7887 14.79 01:38:01.85 +12:08:25.8
140.49124 -49.13618 galactic Psc Second-epoch detections are separated by 2.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1848 Delvaux 0 -0 0 15.0 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:01.85 +12:08:25.8: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:38:01.85 +12:08:25.8: 16.04 +/- 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,2461334.7887,14.79,0.05,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 20261021.2887 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461334.78904882 21.10.2026 06:56:03.818 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 6974
Objects passed selection criteria: 6971
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: 6618.5
Average stars matched: 6553.5 (99.0179 %)
Memory usage VmPeak: 233256 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 01:58:10 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: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461334.78904882 21.10.2026 06:56:03.818 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.10
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: 14 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): 38786
Objects passed selection criteria: 38698
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: 37283.5
Average stars matched: 36312.8 (97.3963 %)
Memory usage VmPeak: 259996 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 01:59:25 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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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: 2461334.78840228
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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 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: 01:46:39.869 +14:00:12.31 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-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Image size: 941.3'x626.7' 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: 01:46:40.646 +14:00:04.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:40.646 +14:00:04.29
Angular distance between the image centers 0.0039 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Image size: 941.3'x626.7' 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: 01:46:38.981 +14:00:36.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:38.981 +14:00:36.81
Angular distance between the image centers 0.0077 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 01:46:40.646 +14:00:04.29
Second-epoch second image center 01:46:38.981 +14:00:36.81
Angular distance between the image centers 0.01127 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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.u361cArQxZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.FMKJ794v5F
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits &> /tmp/tmp.cRyGciTXru
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits &> /tmp/tmp.ud2LqsGRzB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 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 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 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): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950100
a=0.000000 b=1.000000 c=22.950100
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 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 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 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): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=6.0)
Read 6762 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4566 to 34.9567 deg, Dec +8.6053 to +19.2739 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 18.4566 to 34.9567 deg, Dec 8.6053 to 19.2739 deg
Loaded 4732 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): 3812 out of 4016 total matches.
Matched with Tycho-2 4016 out of 6762 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.0 pix Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.1 pix fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
2.1 pix fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Limiting magnitude estimates:
15.6 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.5 mag. Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.3 mag. fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
15.3 mag. fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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.u361cArQxZ (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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=549, bad_region=0, passed=7679
Got 7679 stars (including 7121 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 7679 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
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 493 to 548 (Dec 8.6 to 19.3)
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: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 4873 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4873 sigma_overall_arcsec=0.237 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.223 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.200 n_q1=1261 n_q2=1216 n_q3=1199 n_q4=1197 worst_quadrant_to_overall_ratio=1.365
WCS_HEADER_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits selection=current_pairs N_selected=4873 N_valid=4873 bias_ra_arcsec=0.000 bias_dec_arcsec=0.003 median_sep_arcsec=0.200 p95_sep_arcsec=0.663 n_q1=1261 n_q2=1216 n_q3=1199 n_q4=1197 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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.FMKJ794v5F (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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=519, bad_region=0, passed=6762
Got 6762 stars (including 6236 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 6762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4878 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.239 n_q1=1250 n_q2=1227 n_q3=1200 n_q4=1201 worst_quadrant_to_overall_ratio=1.449
WCS_HEADER_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits selection=current_pairs N_selected=4878 N_valid=4878 bias_ra_arcsec=-0.001 bias_dec_arcsec=0.009 median_sep_arcsec=0.247 p95_sep_arcsec=0.758 n_q1=1250 n_q2=1227 n_q3=1200 n_q4=1201 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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.cRyGciTXru (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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=470, bad_region=0, passed=6139
Got 6139 stars (including 5661 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat
util/solve_plate_with_UCAC5 got 6139 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 492 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 6139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 492 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 6139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 6139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4868 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4868 robust_rms=13.512 arcsec worst_region_rms=27.442 arcsec outer_annulus_rms=27.442 arcsec
SIP_REFIT: SIP order 3 trial: matched=4868 robust_rms=0.486 arcsec worst_region_rms=0.671 arcsec outer_annulus_rms=0.671 arcsec
SIP_REFIT: SIP order 5 trial: matched=4868 robust_rms=0.295 arcsec worst_region_rms=0.337 arcsec outer_annulus_rms=0.288 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4868 robust_rms_before=1.035 arcsec robust_rms_before_corrected=0.300 arcsec robust_rms_after=0.295 arcsec worst_region_rms_before=0.350 worst_region_rms_after=0.337 outer_annulus_rms_before=1.180 outer_annulus_rms_after=0.288
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.350 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits worst_region_rms_kept=0.350 arcsec robust_rms_kept=0.300 arcsec matched=4868
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits N_match=4868 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.317 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.293 sigma_q4_arcsec=0.273 n_q1=1322 n_q2=1163 n_q3=1212 n_q4=1171 worst_quadrant_to_overall_ratio=1.162
WCS_HEADER_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits selection=current_pairs N_selected=4868 N_valid=4868 bias_ra_arcsec=-0.575 bias_dec_arcsec=0.479 median_sep_arcsec=0.907 p95_sep_arcsec=1.911 n_q1=1322 n_q2=1163 n_q3=1212 n_q4=1171 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits -region wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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.ud2LqsGRzB (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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=457, bad_region=0, passed=6049
Got 6049 stars (including 5585 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat
util/solve_plate_with_UCAC5 got 6049 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 492 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 6049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 492 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 6049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 6049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4871 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4871 robust_rms=13.602 arcsec worst_region_rms=27.489 arcsec outer_annulus_rms=27.489 arcsec
SIP_REFIT: SIP order 3 trial: matched=4871 robust_rms=0.493 arcsec worst_region_rms=0.766 arcsec outer_annulus_rms=0.766 arcsec
SIP_REFIT: SIP order 5 trial: matched=4871 robust_rms=0.287 arcsec worst_region_rms=0.322 arcsec outer_annulus_rms=0.292 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4871 robust_rms_before=1.054 arcsec robust_rms_before_corrected=0.291 arcsec robust_rms_after=0.287 arcsec worst_region_rms_before=0.333 worst_region_rms_after=0.322 outer_annulus_rms_before=1.225 outer_annulus_rms_after=0.292
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.333 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits worst_region_rms_kept=0.333 arcsec robust_rms_kept=0.291 arcsec matched=4871
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits N_match=4871 sigma_overall_arcsec=0.299 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.268 sigma_q4_arcsec=0.269 n_q1=1313 n_q2=1156 n_q3=1229 n_q4=1173 worst_quadrant_to_overall_ratio=1.158
WCS_HEADER_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits selection=current_pairs N_selected=4871 N_valid=4871 bias_ra_arcsec=-0.588 bias_dec_arcsec=0.490 median_sep_arcsec=0.923 p95_sep_arcsec=1.937 n_q1=1313 n_q2=1156 n_q3=1229 n_q4=1173 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits -region wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
Saving the final (post-refit) wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits sigma_overall=0.237 worst_q_ratio=1.365
ref2=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits sigma_overall=0.294 worst_q_ratio=1.449
new1=fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits sigma_overall=0.310 worst_q_ratio=1.162
new2=fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits sigma_overall=0.299 worst_q_ratio=1.158
reference average sigma_overall=0.2655 worst_q_ratio=1.407
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_astrometric_residuals.png (4873 matched stars from wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.21 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139_astrometric_residuals.png (4878 matched stars from wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244_astrometric_residuals.png (4868 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245_astrometric_residuals.png (4871 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits'
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:13.55 +10:16:02.9: 11.43 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:14:03.94 +12:47:10.4: 12.50 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:55:37.09 +09:38:08.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:55:37.09 +09:38:08.5: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:13.55 +10:16:02.9: 11.45 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:14:03.94 +12:47:10.4: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter REJECTED candidate at 02:15:13.55 +10:16:02.9: ref_mag=11.44 +/- 0.01 new_mean_mag=11.7661 delta=-0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:14:03.94 +12:47:10.4: ref_mag=12.47 +/- 0.01 new_mean_mag=12.4278 delta=0.05 (need > 0.90)
Adding exclusion_list_local.txt__out20121.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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 20091_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 20091_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20092_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 20092_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 02:13:54.50 +10:28:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20121_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 20121_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20189_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 20189_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 02:10:13.52 +11:31:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20203_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 20203_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 12s
Prepared the HTML report for the field Psc-03-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 ####
01:55:37.09 +09:38:08.5
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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 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: 01:46:39.869 +14:00:12.31 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-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Image size: 941.3'x626.7' 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: 01:46:40.646 +14:00:04.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:40.646 +14:00:04.29
Angular distance between the image centers 0.0039 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Image size: 941.3'x626.7' 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: 01:46:38.981 +14:00:36.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:38.981 +14:00:36.81
Angular distance between the image centers 0.0077 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 01:46:40.646 +14:00:04.29
Second-epoch second image center 01:46:38.981 +14:00:36.81
Angular distance between the image centers 0.01127 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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.WZKoSUPxc4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.iGlqpVgu8j
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits &> /tmp/tmp.5tTjI04bps
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits &> /tmp/tmp.KQSr6dN3Ij
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 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 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 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): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.860050
a=0.000000 b=1.000000 c=22.860050
From vast_summary.log: estimated ref. image limiting mag.: -7.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 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 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 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): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=4.9)
Read 38153 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4016 to 34.9977 deg, Dec +8.5904 to +19.2796 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 18.4016 to 34.9977 deg, Dec 8.5904 to 19.2796 deg
Loaded 4774 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): 3712 out of 4109 total matches.
Matched with Tycho-2 4109 out of 38153 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
1.9 pix Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.0 pix fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
2.0 pix fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Limiting magnitude estimates:
15.8 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.6 mag. Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.5 mag. fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
15.5 mag. fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.6 (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.WZKoSUPxc4 (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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=13, blended=1873, bad_region=4, passed=40626
Got 40626 stars (including 38681 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 40626 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4878 sigma_overall_arcsec=0.229 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.218 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.197 n_q1=1241 n_q2=1253 n_q3=1190 n_q4=1194 worst_quadrant_to_overall_ratio=1.309
WCS_HEADER_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits selection=current_pairs N_selected=4878 N_valid=4878 bias_ra_arcsec=0.005 bias_dec_arcsec=0.005 median_sep_arcsec=0.198 p95_sep_arcsec=0.668 n_q1=1241 n_q2=1253 n_q3=1190 n_q4=1194 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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.iGlqpVgu8j (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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=18, blended=1585, bad_region=24, passed=38135
Got 38135 stars (including 36454 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 38135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 4881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4881 stars left (next iteration limit 5369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4881 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.264 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.238 n_q1=1246 n_q2=1250 n_q3=1199 n_q4=1186 worst_quadrant_to_overall_ratio=1.439
WCS_HEADER_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits selection=current_pairs N_selected=4881 N_valid=4881 bias_ra_arcsec=0.006 bias_dec_arcsec=0.012 median_sep_arcsec=0.242 p95_sep_arcsec=0.737 n_q1=1246 n_q2=1250 n_q3=1199 n_q4=1186 occupied_cells_4x4=16/16
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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.5tTjI04bps (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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=13, blended=1383, bad_region=47, passed=35729
Got 35729 stars (including 34235 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat
util/solve_plate_with_UCAC5 got 35729 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 491 to 549 (Dec 8.3 to 19.4)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 35729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 491 to 549 (Dec 8.3 to 19.4)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 35729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 35729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4872 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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=4872 robust_rms=13.393 arcsec worst_region_rms=27.842 arcsec outer_annulus_rms=27.842 arcsec
SIP_REFIT: SIP order 3 trial: matched=4872 robust_rms=0.481 arcsec worst_region_rms=0.716 arcsec outer_annulus_rms=0.716 arcsec
SIP_REFIT: SIP order 5 trial: matched=4872 robust_rms=0.288 arcsec worst_region_rms=0.328 arcsec outer_annulus_rms=0.286 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4872 robust_rms_before=1.030 arcsec robust_rms_before_corrected=0.293 arcsec robust_rms_after=0.288 arcsec worst_region_rms_before=0.339 worst_region_rms_after=0.328 outer_annulus_rms_before=1.173 outer_annulus_rms_after=0.286
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.339 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits worst_region_rms_kept=0.339 arcsec robust_rms_kept=0.293 arcsec matched=4872
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits N_match=4872 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.313 sigma_q2_arcsec=0.344 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.263 n_q1=1333 n_q2=1180 n_q3=1208 n_q4=1151 worst_quadrant_to_overall_ratio=1.156
WCS_HEADER_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits selection=current_pairs N_selected=4872 N_valid=4872 bias_ra_arcsec=-0.573 bias_dec_arcsec=0.493 median_sep_arcsec=0.904 p95_sep_arcsec=1.899 n_q1=1333 n_q2=1180 n_q3=1208 n_q4=1151 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits -region wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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.KQSr6dN3Ij (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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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=10, blended=1394, bad_region=48, passed=35657
Got 35657 stars (including 34147 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat
util/solve_plate_with_UCAC5 got 35657 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 491 to 549 (Dec 8.4 to 19.4)
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: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 35657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 491 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4875 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(), 35657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 35657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4870 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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=13.501 arcsec worst_region_rms=28.346 arcsec outer_annulus_rms=28.346 arcsec
SIP_REFIT: SIP order 3 trial: matched=4870 robust_rms=0.490 arcsec worst_region_rms=0.818 arcsec outer_annulus_rms=0.818 arcsec
SIP_REFIT: SIP order 5 trial: matched=4870 robust_rms=0.280 arcsec worst_region_rms=0.318 arcsec outer_annulus_rms=0.291 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4870 robust_rms_before=1.051 arcsec robust_rms_before_corrected=0.283 arcsec robust_rms_after=0.280 arcsec worst_region_rms_before=0.321 worst_region_rms_after=0.318 outer_annulus_rms_before=1.236 outer_annulus_rms_after=0.291
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.321 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits worst_region_rms_kept=0.321 arcsec robust_rms_kept=0.283 arcsec matched=4870
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits N_match=4870 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.256 n_q1=1329 n_q2=1184 n_q3=1206 n_q4=1151 worst_quadrant_to_overall_ratio=1.158
WCS_HEADER_DIAG: file=fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits selection=current_pairs N_selected=4870 N_valid=4870 bias_ra_arcsec=-0.591 bias_dec_arcsec=0.498 median_sep_arcsec=0.922 p95_sep_arcsec=1.932 n_q1=1329 n_q2=1184 n_q3=1206 n_q4=1151 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits -region wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-55-07_20.00sec_-0.00C_LIGHTs_0244.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.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_2026-10-21_CI_Psc-03-Q1b1x1_015657_TTUQ1b1x1_2330511_lzEAQ2Hh/wcs_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245.fits
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:23:17.27 +16:32:18.2: 13.75 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:14.63 +14:03:16.3: 14.72 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:55.76 +18:59:51.3: 13.99 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:17:53.92 +14:29:52.0: 14.57 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:58.38 +14:42:23.7: 14.73 +/- 0.12 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:52.58 +18:28:27.2: 14.03 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:36:18.91 +18:57:43.0: 14.25 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:18:45.13 +15:31:49.9: 14.15 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:50:52.58 +18:28:27.2: 14.06 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:19:58.38 +14:42:23.7: 14.76 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:23:17.27 +16:32:18.2: 13.82 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:18:45.13 +15:31:49.9: 14.10 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:36:18.91 +18:57:43.0: 14.32 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:55.76 +18:59:51.3: 14.06 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:36:05.69 +14:36:53.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:17:53.92 +14:29:52.0: 14.68 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:19:14.63 +14:03:16.3: 14.77 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Forced photometry filter REJECTED candidate at 01:50:52.58 +18:28:27.2: ref_mag=14.04 +/- 0.04 new_mean_mag=14.5630 delta=-0.52 (need > 0.90)
Forced photometry reference-image weighted average: 14.28 +/- 0.05
Forced photometry filter REJECTED candidate at 01:23:17.27 +16:32:18.2: ref_mag=13.78 +/- 0.04 new_mean_mag=14.1685 delta=-0.39 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:19:58.38 +14:42:23.7: ref_mag=14.74 +/- 0.09 new_mean_mag=14.4321 delta=0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:18:45.13 +15:31:49.9: ref_mag=14.13 +/- 0.05 new_mean_mag=14.2045 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Forced photometry reference-image weighted average: 14.01 +/- 0.04
Forced photometry reference-image weighted average: 14.61 +/- 0.08
Forced photometry filter REJECTED candidate at 01:36:18.91 +18:57:43.0: ref_mag=14.28 +/- 0.05 new_mean_mag=14.6365 delta=-0.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:31:55.76 +18:59:51.3: ref_mag=14.01 +/- 0.04 new_mean_mag=14.2071 delta=-0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:19:14.63 +14:03:16.3: ref_mag=14.74 +/- 0.09 new_mean_mag=14.3959 delta=0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:17:53.92 +14:29:52.0: ref_mag=14.61 +/- 0.08 new_mean_mag=14.5443 delta=0.07 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:15.44 +14:04:39.9: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:36:05.69 +14:36:53.7: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter REJECTED candidate at 01:36:05.69 +14:36:53.7: ref_mag=12.74 +/- 0.01 new_mean_mag=13.0209 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:53.26 +09:15:44.1: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:14:13.89 +10:03:38.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:16:36.77 +13:36:24.5: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:44.33 +11:22:31.0: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:20:45.92 +16:44:51.0: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:30:15.44 +14:04:39.9: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:49:59.07 +11:14:56.0: 14.09 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:42:53.26 +09:15:44.1: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:14:13.89 +10:03:38.8: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:16:36.77 +13:36:24.5: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:44.33 +11:22:31.0: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:20:45.92 +16:44:51.0: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:08.65 +13:27:09.5: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:33.26 +11:19:30.9: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:49:59.07 +11:14:56.0: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Forced photometry filter REJECTED candidate at 01:49:59.07 +11:14:56.0: ref_mag=13.98 +/- 0.04 new_mean_mag=14.1077 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:04:03.06 +18:51:36.9: 14.32 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:52:08.65 +13:27:09.5: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:33.26 +11:19:30.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:04:03.06 +18:51:36.9: 14.31 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.06
Forced photometry filter REJECTED candidate at 02:04:03.06 +18:51:36.9: ref_mag=14.31 +/- 0.06 new_mean_mag=14.5688 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:35.32 +10:17:00.2: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:40:35.32 +10:17:00.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:24.83 +13:43:17.2: 14.48 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:24.83 +13:43:17.2: 14.53 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.06
Forced photometry filter REJECTED candidate at 01:39:24.83 +13:43:17.2: ref_mag=14.50 +/- 0.06 new_mean_mag=14.5917 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:05:48.97 +18:38:40.7: 14.95 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:05:48.97 +18:38:40.7: 14.80 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.10
Forced photometry filter REJECTED candidate at 02:05:48.97 +18:38:40.7: ref_mag=14.87 +/- 0.10 new_mean_mag=14.7339 delta=0.14 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:25.24 +16:56:07.5: 14.86 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:30:25.24 +16:56:07.5: 14.91 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.10
Forced photometry filter REJECTED candidate at 01:30:25.24 +16:56:07.5: ref_mag=14.88 +/- 0.10 new_mean_mag=14.6850 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:01.85 +12:08:25.8: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:38:01.85 +12:08:25.8: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:52.16 +13:46:28.9: 14.64 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:24:52.90 +16:38:45.9: 15.17 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:24:52.02 +10:02:42.1: 15.19 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:51:43.82 +17:44:25.2: 14.70 +/- 0.10 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:17.79 +15:49:48.9: 15.38 +/- 0.23 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:25.38 +14:16:58.0: 14.97 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:52.16 +13:46:28.9: 14.85 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.07
Forced photometry filter REJECTED candidate at 01:45:52.16 +13:46:28.9: ref_mag=14.71 +/- 0.07 new_mean_mag=14.8017 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:24:52.02 +10:02:42.1: 15.31 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.14
Forced photometry filter REJECTED candidate at 01:24:52.02 +10:02:42.1: ref_mag=15.24 +/- 0.14 new_mean_mag=14.8252 delta=0.41 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:46:15.05 +11:58:32.5: 15.27 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:24:52.90 +16:38:45.9: 15.27 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.13
Forced photometry filter REJECTED candidate at 01:24:52.90 +16:38:45.9: ref_mag=15.21 +/- 0.13 new_mean_mag=14.8831 delta=0.33 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:51:43.82 +17:44:25.2: 15.02 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:16:17.79 +15:49:48.9: 15.49 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.08
Forced photometry reference-image weighted average: 15.42 +/- 0.18
Forced photometry filter REJECTED candidate at 01:51:43.82 +17:44:25.2: ref_mag=14.81 +/- 0.08 new_mean_mag=14.9554 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:16:17.79 +15:49:48.9: ref_mag=15.42 +/- 0.18 new_mean_mag=14.9192 delta=0.50 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:19:25.38 +14:16:58.0: 15.46 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.14
Forced photometry filter REJECTED candidate at 01:19:25.38 +14:16:58.0: ref_mag=15.09 +/- 0.14 new_mean_mag=14.9011 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:41.99 +12:36:41.4: 15.00 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:06.88 +18:57:30.0: 15.35 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:46:15.05 +11:58:32.5: 15.35 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.30 +/- 0.12
Forced photometry filter REJECTED candidate at 01:46:15.05 +11:58:32.5: ref_mag=15.30 +/- 0.12 new_mean_mag=15.0049 delta=0.30 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:09.44 +18:45:21.3: 14.87 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:05.05 +18:16:05.9: 15.51 +/- 0.25 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:17.06 +15:32:46.0: 15.65 +/- 0.23 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:33:40.51 +10:25:24.3: 15.62 +/- 0.25 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:23:36.87 +12:18:12.6: 15.41 +/- 0.22 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:16:41.99 +12:36:41.4: 14.85 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:25:10.83 +12:59:16.3: 14.82 +/- 0.12 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:06.88 +18:57:30.0: 15.37 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.11
Forced photometry reference-image weighted average: 15.36 +/- 0.14
Forced photometry filter REJECTED candidate at 01:16:41.99 +12:36:41.4: ref_mag=14.93 +/- 0.11 new_mean_mag=14.8215 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:39:06.88 +18:57:30.0: ref_mag=15.36 +/- 0.14 new_mean_mag=14.9399 delta=0.42 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:09.44 +18:45:21.3: 15.21 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.11
Forced photometry filter REJECTED candidate at 01:34:09.44 +18:45:21.3: ref_mag=14.97 +/- 0.11 new_mean_mag=14.9720 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:23:36.87 +12:18:12.6: 15.00 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:19:05.05 +18:16:05.9: 15.09 +/- 0.21 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:33:40.51 +10:25:24.3: 15.09 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:17.06 +15:32:46.0: 15.38 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.13
Forced photometry reference-image weighted average: 15.26 +/- 0.16
Forced photometry filter REJECTED candidate at 01:23:36.87 +12:18:12.6: ref_mag=15.16 +/- 0.13 new_mean_mag=15.0716 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 15.50 +/- 0.15
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:25:10.83 +12:59:16.3: 14.87 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.14
Forced photometry filter REJECTED candidate at 01:19:05.05 +18:16:05.9: ref_mag=15.26 +/- 0.16 new_mean_mag=15.0310 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:34:17.06 +15:32:46.0: ref_mag=15.50 +/- 0.15 new_mean_mag=15.0760 delta=0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:33:40.51 +10:25:24.3: ref_mag=15.27 +/- 0.14 new_mean_mag=15.0394 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 14.84 +/- 0.09
Forced photometry filter REJECTED candidate at 01:25:10.83 +12:59:16.3: ref_mag=14.84 +/- 0.09 new_mean_mag=14.9086 delta=-0.07 (need > 0.90)
Adding exclusion_list_local.txt__out51862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52518.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 7s
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Considering the candidate 51672_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51672_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51674_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51674_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51675_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51675_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:26:20.54 +17:42:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51676_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51676_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51678_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51678_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51679_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51679_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51683_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51683_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:23:30.60 +11:17:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51686_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51686_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51687_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51687_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51689_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51689_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51690_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51690_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:45:28.88 +17:08:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51692_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51692_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:28:03.46 +10:55:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51693_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51693_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 51723_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 51723_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:55:37.09 +09:38:08.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51862_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 51862_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 51913_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 51913_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 51948_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 51948_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52031_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 52031_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52047_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52047_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:47:13.26 +17:54:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52054_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 52054_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52096_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52096_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:39:44.53 +16:26:02.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52157_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 52157_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52181_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52181_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:44:30.98 +14:02:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52207_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52207_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52223_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52223_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 02:07:33.09 +12:06:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52245_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52245_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 01:43:42.54 +12:53:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52248_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52248_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
**** FOUND 02:02:43.05 +13:27:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52276_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 52276_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52311_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 52311_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52391_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52391_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52427_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 52427_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52474_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52474_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52480_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52480_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52486_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52486_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52518_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
Preparing report for the candidate 52518_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
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Considering the candidate 52522_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52522_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52545_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52545_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52548_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52548_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52593_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52593_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52594_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52594_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52607_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52607_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52619_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52619_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52625_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52625_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52627_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52627_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52634_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52634_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52652_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52652_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52658_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52658_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52675_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52675_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52690_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52690_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 52696_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 52696_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
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Considering the candidate 09160_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245
The candidate 09160_fd_Psc-03-Q1b1x1_2026-10-21_01-56-03_20.00sec_0.00C_LIGHTs_0245 did not pass the final checks
