This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz
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 06.2398 2461319.7398 11.44 23:06:33.79 -03:40:10.1
71.47720 -55.68669 galactic Aqr Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.236 Honoria 0 0 0 11.3 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:06:33.79 -03:40:10.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:06:33.79 -03:40:10.1: 15.74 +/- 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,2461319.7398,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 06.2398 2461319.7398 12.49 23:32:03.34 -04:48:04.8
79.14286 -60.73422 galactic Aqr Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.317 Roxane -0 -0 0 12.3 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:03.34 -04:48:04.8: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:03.34 -04:48:04.8: 15.61 +/- 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,2461319.7398,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 12.49CV 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 06.2398 2461319.7398 13.47 23:20:40.31 -02:10:34.9
78.01325 -56.91091 galactic Psc Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.570 Kythera -0 -0 0 13.5 0 0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:20:40.31 -02:10:34.9: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:20:40.31 -02:10:34.9: 15.84 +/- 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,2461319.7398,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 13.47CV 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 06.2398 2461319.7398 13.46 23:20:11.08 -01:55:59.0
78.11940 -56.64514 galactic Psc Second-epoch detections are separated by 1.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.328 Gudrun 0 0 0 13.7 0 0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:20:11.08 -01:55:59.0: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:20:11.08 -01:55:59.0: 15.82 +/- 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,2461319.7398,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 13.46CV 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 06.2398 2461319.7398 13.53 23:16:29.50 -03:50:10.6
74.55950 -57.49907 galactic Aqr Second-epoch detections are separated by 1.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.788 Hohensteina 0 -0 0 13.9 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:16:29.50 -03:50:10.6: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:16:29.50 -03:50:10.6: 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!
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,2461319.7398,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 06.2398 2461319.7398 13.97 23:22:00.01 -06:13:33.1
73.40622 -60.18911 galactic Aqr Second-epoch detections are separated by 0.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.799 Gudula -0 1 1 13.8 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:22:00.01 -06:13:33.1: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:22:00.01 -06:13:33.1: 15.67 +/- 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,2461319.7398,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 13.97CV 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 06.2398 2461319.7398 14.33 23:15:02.34 -01:16:39.8
77.08198 -55.32366 galactic Psc Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.673 Edda 0 -0 0 14.3 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:15:02.34 -01:16:39.8: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:15:02.34 -01:16:39.8: 15.86 +/- 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,2461319.7398,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 06.2398 2461319.7398 14.45 23:07:31.34 -00:25:45.3
75.56329 -53.46114 galactic Psc Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1157 Arabia 0 1 1 14.5 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:07:31.34 -00:25:45.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:07:31.34 -00:25:45.3: 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,2461319.7398,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 14.45CV 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 06.2398 2461319.7398 14.61 23:17:55.64 -01:45:43.5
77.52346 -56.15666 galactic Psc Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.440 Theodora 0 -0 0 14.6 0 0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:17:55.64 -01:45:43.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:17:55.64 -01:45:43.5: 15.82 +/- 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,2461319.7398,14.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.2398 14.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
First image: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Last image: 2461319.74013914 06.10.2026 05:45:38.022 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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.: -7.34
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 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): 5220
Objects passed selection criteria: 5219
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: 4997.25
Average stars matched: 4773 (95.5125 %)
Memory usage VmPeak: 232492 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Oct 4 15:05:03 CDT 2026
VaST build number 1.0rc89-232-g1547b37e
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-04)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Oct 6 01:05:49 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: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
First image: 2461242.93564273 21.07.2026 10:27:09.532 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Last image: 2461319.74013914 06.10.2026 05:45:38.022 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 120
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.06
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: 106 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): 29320
Objects passed selection criteria: 29249
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: 28523.2
Average stars matched: 27034.8 (94.7815 %)
Memory usage VmPeak: 255456 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Oct 4 15:05:03 CDT 2026
VaST build number 1.0rc89-232-g1547b37e
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-04)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Oct 6 01:09:21 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.cat to cache
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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: 2461319.73948134
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits exists and is non-empty
wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (1st reference image)
verification OK: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:34.580 -02:00:27.91 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits (1st new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:34.599 -01:59:19.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:34.599 -01:59:19.65
Angular distance between the image centers 0.0190 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits (2nd new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:31.824 -01:59:47.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:31.824 -01:59:47.94
Angular distance between the image centers 0.0160 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 23:08:34.599 -01:59:19.65
Second-epoch second image center 23:08:31.824 -01:59:47.94
Angular distance between the image centers 0.01397 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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits &> /tmp/tmp.CkmW1GZaSz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits &> /tmp/tmp.rxwgqAv6pu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits &> /tmp/tmp.q7QObvuDzE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits &> /tmp/tmp.j2fI8c6osq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
The reference image (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits) and catalog (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat) found
'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat' -> 'wcsmag.cat'
Read 6415 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2860 to 355.0261 deg, Dec -7.2671 to +3.2586 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 339.2860 to 355.0261 deg, Dec -7.2671 to 3.2586 deg
Loaded 4387 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): 3702 out of 3810 total matches.
Matched with Tycho-2 3810 out of 6415 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.655300
a=0.000000 b=1.000000 c=22.655300
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6415 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2860 to 355.0261 deg, Dec -7.2671 to +3.2586 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 339.2860 to 355.0261 deg, Dec -7.2671 to 3.2586 deg
Loaded 4387 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): 3702 out of 3810 total matches.
Matched with Tycho-2 3810 out of 6415 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (aperture=6.3)
Read 6260 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2725 to 355.0121 deg, Dec -7.2776 to +3.2517 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 339.2725 to 355.0121 deg, Dec -7.2776 to 3.2517 deg
Loaded 4385 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): 3695 out of 3795 total matches.
Matched with Tycho-2 3795 out of 6260 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
cp: cannot create regular file 'local_wcs_cache/': Not a directory
Median FWHM seeing for isolated stars:
2.3 pix Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
2.2 pix Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
2.3 pix fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
2.3 pix fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Limiting magnitude estimates:
15.3 mag. Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
15.3 mag. Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
15.4 mag. fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
15.4 mag. fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
All-image limiting magnitude estimate: 15.4 (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
############ /tmp/tmp.CkmW1GZaSz (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=388, bad_region=1637, passed=6415
Got 6415 stars (including 4478 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
util/solve_plate_with_UCAC5 got 6415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4346 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4337 matched stars entering correct_measured_positions(), 4337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4337 matched stars entering correct_measured_positions(), 5064 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4346 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 5064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4338 matched stars entering correct_measured_positions(), 5064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4338 stars left (next iteration limit 4770)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits N_match=4338 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.299 sigma_q4_arcsec=0.295 n_q1=1429 n_q2=758 n_q3=1353 n_q4=798 worst_quadrant_to_overall_ratio=1.040
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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.rxwgqAv6pu (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=360, bad_region=1607, passed=6260
Got 6260 stars (including 4361 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
util/solve_plate_with_UCAC5 got 6260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4238 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4238 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4230 matched stars entering correct_measured_positions(), 4940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4230 stars left (next iteration limit 4653)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits N_match=4230 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.382 sigma_q4_arcsec=0.346 n_q1=1416 n_q2=724 n_q3=1303 n_q4=787 worst_quadrant_to_overall_ratio=1.062
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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.q7QObvuDzE (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=421, bad_region=1754, passed=7090
Got 7090 stars (including 5003 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 7090 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4854 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 4846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 5678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4855 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 5678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 5678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4847 stars left (next iteration limit 5330)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4847 robust_rms=7.751 arcsec worst_region_rms=16.030 arcsec outer_annulus_rms=16.030 arcsec
SIP_REFIT: SIP order 3 trial: matched=4847 robust_rms=0.392 arcsec worst_region_rms=0.585 arcsec outer_annulus_rms=0.585 arcsec
SIP_REFIT: SIP order 5 trial: matched=4847 robust_rms=0.323 arcsec worst_region_rms=0.405 arcsec outer_annulus_rms=0.405 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4847 robust_rms_before=0.926 arcsec robust_rms_before_corrected=0.323 arcsec robust_rms_after=0.323 arcsec worst_region_rms_before=0.417 worst_region_rms_after=0.405 outer_annulus_rms_before=0.923 outer_annulus_rms_after=0.405
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.417 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits worst_region_rms_kept=0.417 arcsec robust_rms_kept=0.323 arcsec matched=4847
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits N_match=4847 sigma_overall_arcsec=0.343 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.356 n_q1=1591 n_q2=908 n_q3=1460 n_q4=888 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits -region wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.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.j2fI8c6osq (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=396, bad_region=1741, passed=7106
Got 7106 stars (including 5050 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat
util/solve_plate_with_UCAC5 got 7106 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4859 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 4854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 5696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4860 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 5696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 5696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4855 stars left (next iteration limit 5339)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4855 robust_rms=7.763 arcsec worst_region_rms=15.291 arcsec outer_annulus_rms=15.291 arcsec
SIP_REFIT: SIP order 3 trial: matched=4855 robust_rms=0.368 arcsec worst_region_rms=0.594 arcsec outer_annulus_rms=0.594 arcsec
SIP_REFIT: SIP order 5 trial: matched=4855 robust_rms=0.300 arcsec worst_region_rms=0.390 arcsec outer_annulus_rms=0.390 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4855 robust_rms_before=0.912 arcsec robust_rms_before_corrected=0.301 arcsec robust_rms_after=0.300 arcsec worst_region_rms_before=0.400 worst_region_rms_after=0.390 outer_annulus_rms_before=0.903 outer_annulus_rms_after=0.390
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.400 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits worst_region_rms_kept=0.400 arcsec robust_rms_kept=0.301 arcsec matched=4855
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits N_match=4855 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.308 sigma_q4_arcsec=0.325 n_q1=1594 n_q2=892 n_q3=1482 n_q4=887 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits -region wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits to local_wcs_cache/
'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits' -> 'local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits'
Saving the final (post-refit) wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits to local_wcs_cache/
'wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits' -> 'local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits'
Saving the final (post-refit) wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits to local_wcs_cache/
'wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits' -> 'local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits'
Saving the final (post-refit) wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits to local_wcs_cache/
'wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits' -> 'local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits sigma_overall=0.314 worst_q_ratio=1.040
ref2=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits sigma_overall=0.379 worst_q_ratio=1.062
new1=fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits sigma_overall=0.343 worst_q_ratio=1.070
new2=fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits sigma_overall=0.316 worst_q_ratio=1.049
reference average sigma_overall=0.3465 worst_q_ratio=1.051
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017_astrometric_residuals.png (4338 matched stars from wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018_astrometric_residuals.png (4230 matched stars from wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266_astrometric_residuals.png (4847 matched stars from wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267_astrometric_residuals.png (4855 matched stars from wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits'
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits'
Preparing the HTML report for the field Psc-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:21:26.74 -03:04:03.1: 11.58 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:01:58.97 +00:24:25.2: 12.00 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:06:33.79 -03:40:10.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:09:52.91 -01:53:07.8: 12.23 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:07:13.48 -01:29:21.6: 12.06 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 22:59:24.11 -02:53:06.1: 12.07 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:06:33.79 -03:40:10.1: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:01:58.97 +00:24:25.2: 11.99 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:59:24.11 -02:53:06.1: 12.05 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:07:13.48 -01:29:21.6: 12.07 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:21:26.74 -03:04:03.1: 11.57 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:09:52.91 -01:53:07.8: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 23:01:58.97 +00:24:25.2: ref_mag=12.00 +/- 0.01 new_mean_mag=11.9938 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:21:26.74 -03:04:03.1: ref_mag=11.57 +/- 0.01 new_mean_mag=11.7720 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:09:52.91 -01:53:07.8: ref_mag=12.23 +/- 0.01 new_mean_mag=12.2049 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter REJECTED candidate at 22:59:24.11 -02:53:06.1: ref_mag=12.06 +/- 0.01 new_mean_mag=12.1139 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:07:13.48 -01:29:21.6: ref_mag=12.06 +/- 0.01 new_mean_mag=12.0869 delta=-0.02 (need > 0.90)
Adding exclusion_list_local.txt__out20215.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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 20215_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 20215_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20218_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 20218_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20219_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 20219_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20220_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 20220_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20221_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 20221_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20225_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 20225_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Psc-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:06:33.79 -03:40:10.1
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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.cat to cache
SExtractor catalog cache: saved Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Creating symlink local_wcs_cache/wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits exists and is non-empty
wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (1st reference image)
verification OK: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:34.580 -02:00:27.91 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits (1st new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:34.599 -01:59:19.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:34.599 -01:59:19.65
Angular distance between the image centers 0.0190 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits (2nd new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:08:31.824 -01:59:47.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:08:34.580 -02:00:27.91
Second-epoch image center 23:08:31.824 -01:59:47.94
Angular distance between the image centers 0.0160 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 23:08:34.599 -01:59:19.65
Second-epoch second image center 23:08:31.824 -01:59:47.94
Angular distance between the image centers 0.01397 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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits &> /tmp/tmp.g3l6CcJzJW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits &> /tmp/tmp.Q0iK6xxPRt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits &> /tmp/tmp.f4PVq62PvU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits &> /tmp/tmp.PSIPSMYwBx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Found non-empty wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits and wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
The reference image (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits) and catalog (wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat) found
'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat' -> 'wcsmag.cat'
Read 35879 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2853 to 355.0336 deg, Dec -7.2742 to +3.2602 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 339.2853 to 355.0336 deg, Dec -7.2742 to 3.2602 deg
Loaded 4394 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3591 out of 3893 total matches.
Matched with Tycho-2 3893 out of 35879 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.537600
a=0.000000 b=1.000000 c=22.537600
From vast_summary.log: estimated ref. image limiting mag.: -7.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 35879 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2853 to 355.0336 deg, Dec -7.2742 to +3.2602 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 339.2853 to 355.0336 deg, Dec -7.2742 to 3.2602 deg
Loaded 4394 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3591 out of 3893 total matches.
Matched with Tycho-2 3893 out of 35879 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (aperture=4.9)
Read 36137 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 339.2724 to 355.0227 deg, Dec -7.2779 to +3.2557 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 339.2724 to 355.0227 deg, Dec -7.2779 to 3.2557 deg
Loaded 4393 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): 3594 out of 3890 total matches.
Matched with Tycho-2 3890 out of 36137 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Forced-photometry filter: calibrated wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -> calib.txt_param_ref_wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 65 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
2.1 pix Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
2.2 pix fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
2.2 pix fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Limiting magnitude estimates:
15.5 mag. Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
15.5 mag. Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
15.6 mag. fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
15.6 mag. fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
All-image limiting magnitude estimate: 15.6 (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.g3l6CcJzJW (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=1717, bad_region=7702, passed=35853
Got 35853 stars (including 26731 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat
util/solve_plate_with_UCAC5 got 35853 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 29872 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 29872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 29872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4852 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits N_match=4852 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.299 n_q1=1558 n_q2=904 n_q3=1485 n_q4=905 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.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.Q0iK6xxPRt (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits' -> 'wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS_IMAGE_NAME=wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS-calibrated image found: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
Checking if the catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits alredy exist and is non-empty...
Catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat corresponding to the image wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits
WCS catalog name: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=8, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1465, bad_region=7825, passed=36110
Got 36110 stars (including 27137 good ones) from the SExtractor catalog wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat
util/solve_plate_with_UCAC5 got 36110 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 4854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 30009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 30009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 30009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4854 stars left (next iteration limit 5339)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits N_match=4854 sigma_overall_arcsec=0.372 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.355 n_q1=1577 n_q2=898 n_q3=1478 n_q4=901 worst_quadrant_to_overall_ratio=1.095
The image catalog is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits -region wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.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.f4PVq62PvU (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=9, blended=1862, bad_region=6708, passed=36010
Got 36010 stars (including 28139 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 36010 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 30803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 30803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 30803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4835 stars left (next iteration limit 5318)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.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=4835 robust_rms=7.526 arcsec worst_region_rms=15.131 arcsec outer_annulus_rms=15.131 arcsec
SIP_REFIT: SIP order 3 trial: matched=4835 robust_rms=0.388 arcsec worst_region_rms=0.634 arcsec outer_annulus_rms=0.634 arcsec
SIP_REFIT: SIP order 5 trial: matched=4835 robust_rms=0.317 arcsec worst_region_rms=0.397 arcsec outer_annulus_rms=0.397 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4835 robust_rms_before=0.924 arcsec robust_rms_before_corrected=0.316 arcsec robust_rms_after=0.317 arcsec worst_region_rms_before=0.414 worst_region_rms_after=0.397 outer_annulus_rms_before=0.914 outer_annulus_rms_after=0.397
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.414 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits worst_region_rms_kept=0.414 arcsec robust_rms_kept=0.316 arcsec matched=4835
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits N_match=4835 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.350 n_q1=1616 n_q2=854 n_q3=1516 n_q4=849 worst_quadrant_to_overall_ratio=1.066
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits -region wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.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.PSIPSMYwBx (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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=3, blended=1835, bad_region=6664, passed=35937
Got 35937 stars (including 28101 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat
util/solve_plate_with_UCAC5 got 35937 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 4829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 30773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 30773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 30773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4829 stars left (next iteration limit 5311)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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=4829 robust_rms=7.482 arcsec worst_region_rms=15.212 arcsec outer_annulus_rms=15.212 arcsec
SIP_REFIT: SIP order 3 trial: matched=4829 robust_rms=0.368 arcsec worst_region_rms=0.636 arcsec outer_annulus_rms=0.636 arcsec
SIP_REFIT: SIP order 5 trial: matched=4829 robust_rms=0.297 arcsec worst_region_rms=0.391 arcsec outer_annulus_rms=0.391 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4829 robust_rms_before=0.914 arcsec robust_rms_before_corrected=0.296 arcsec robust_rms_after=0.297 arcsec worst_region_rms_before=0.418 worst_region_rms_after=0.391 outer_annulus_rms_before=0.912 outer_annulus_rms_after=0.391
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.418 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits worst_region_rms_kept=0.418 arcsec robust_rms_kept=0.296 arcsec matched=4829
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits N_match=4829 sigma_overall_arcsec=0.311 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.299 sigma_q4_arcsec=0.322 n_q1=1615 n_q2=858 n_q3=1499 n_q4=857 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits -region wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-44-41_20.00sec_-0.00C_LIGHT_0266.fits
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.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_2026-10-06_CI_Psc-09-Q2b1x1_005343_TTUQ2b1x1_1471515_vPzJ7XZz/wcs_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267.fits
Preparing the HTML report for the field Psc-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:22.12 -04:43:34.4: 14.96 +/- 0.20 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:32.69 -01:07:36.2: 14.43 +/- 0.11 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:33:02.62 +01:48:14.2: 14.56 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 22:53:54.94 +01:29:31.7: 14.95 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:27.71 +01:56:30.2: 14.44 +/- 0.10 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:36.20 -03:37:39.0: 14.81 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:40.84 -02:03:29.6: 14.93 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:29:46.10 -00:30:59.2: 13.93 +/- 0.07 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 22:51:11.46 +01:59:38.1: 14.36 +/- 0.09 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:21:34.51 -05:38:40.5: 14.48 +/- 0.12 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:29:46.10 -00:30:59.2: 14.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter REJECTED candidate at 23:29:46.10 -00:30:59.2: ref_mag=14.00 +/- 0.05 new_mean_mag=14.3406 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:27.71 +01:56:30.2: 14.47 +/- 0.11 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:53:54.94 +01:29:31.7: 14.88 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.07
Forced photometry filter REJECTED candidate at 23:24:27.71 +01:56:30.2: ref_mag=14.45 +/- 0.07 new_mean_mag=14.7749 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:36.20 -03:37:39.0: 15.30 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.10
Forced photometry filter REJECTED candidate at 22:53:54.94 +01:29:31.7: ref_mag=14.91 +/- 0.10 new_mean_mag=14.8652 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.95 +/- 0.15
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:21:34.51 -05:38:40.5: 14.46 +/- 0.12 detection
Forced photometry filter REJECTED candidate at 23:34:36.20 -03:37:39.0: ref_mag=14.95 +/- 0.15 new_mean_mag=14.8000 delta=0.15 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:22.12 -04:43:34.4: 14.91 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:40.84 -02:03:29.6: 14.66 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.09
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:32.69 -01:07:36.2: 14.52 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.13
Forced photometry filter REJECTED candidate at 23:21:34.51 -05:38:40.5: ref_mag=14.47 +/- 0.09 new_mean_mag=14.5440 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:51:11.46 +01:59:38.1: 14.48 +/- 0.10 detection
Forced photometry filter REJECTED candidate at 23:28:22.12 -04:43:34.4: ref_mag=14.93 +/- 0.13 new_mean_mag=14.6965 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.76 +/- 0.11
Forced photometry filter REJECTED candidate at 23:26:40.84 -02:03:29.6: ref_mag=14.76 +/- 0.11 new_mean_mag=14.8096 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:33:02.62 +01:48:14.2: 14.49 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.07
Forced photometry reference-image weighted average: 14.47 +/- 0.08
Forced photometry filter REJECTED candidate at 23:28:32.69 -01:07:36.2: ref_mag=14.47 +/- 0.08 new_mean_mag=14.6842 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:51:11.46 +01:59:38.1: ref_mag=14.41 +/- 0.07 new_mean_mag=14.5497 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 14.52 +/- 0.09
Forced photometry filter REJECTED candidate at 23:33:02.62 +01:48:14.2: ref_mag=14.52 +/- 0.09 new_mean_mag=14.4163 delta=0.11 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:38.14 -05:12:46.5: 13.03 +/- 0.04 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:03.34 -04:48:04.8: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:14:52.06 -01:03:12.3: 12.49 +/- 0.02 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:17:48.03 -03:15:44.8: 13.78 +/- 0.05 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:24:17.14 -06:14:03.4: 13.25 +/- 0.04 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:17:24.03 +00:13:44.8: 13.03 +/- 0.03 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:16:29.50 -03:50:10.6: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:20:11.08 -01:55:59.0: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:20:40.31 -02:10:34.9: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:38.14 -05:12:46.5: 13.07 +/- 0.04 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:17:48.03 -03:15:44.8: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Forced photometry filter REJECTED candidate at 23:17:48.03 -03:15:44.8: ref_mag=13.80 +/- 0.04 new_mean_mag=14.1604 delta=-0.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:26:38.14 -05:12:46.5: ref_mag=13.05 +/- 0.03 new_mean_mag=13.0402 delta=0.01 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:17:24.03 +00:13:44.8: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter REJECTED candidate at 23:17:24.03 +00:13:44.8: ref_mag=13.03 +/- 0.02 new_mean_mag=13.0982 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:16:29.50 -03:50:10.6: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:14:52.06 -01:03:12.3: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 23:14:52.06 -01:03:12.3: ref_mag=12.49 +/- 0.01 new_mean_mag=12.6189 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:20:11.08 -01:55:59.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:20:40.31 -02:10:34.9: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:22:00.01 -06:13:33.1: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:03.34 -04:48:04.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:24:17.14 -06:14:03.4: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter REJECTED candidate at 23:24:17.14 -06:14:03.4: ref_mag=13.26 +/- 0.03 new_mean_mag=13.5004 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:22:00.01 -06:13:33.1: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:06.29 +00:02:55.6: 13.94 +/- 0.07 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:29:29.36 -00:58:10.7: 14.31 +/- 0.10 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:15:02.34 -01:16:39.8: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:43.57 -02:57:42.9: 14.72 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:29:29.36 -00:58:10.7: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Forced photometry filter REJECTED candidate at 23:29:29.36 -00:58:10.7: ref_mag=14.18 +/- 0.06 new_mean_mag=14.2334 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:06.29 +00:02:55.6: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry filter REJECTED candidate at 23:32:06.29 +00:02:55.6: ref_mag=13.94 +/- 0.05 new_mean_mag=14.1791 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:21:22.49 -03:24:13.9: 14.21 +/- 0.09 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:15:02.34 -01:16:39.8: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:43.57 -02:57:42.9: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Forced photometry filter REJECTED candidate at 23:35:43.57 -02:57:42.9: ref_mag=14.69 +/- 0.11 new_mean_mag=14.4609 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:21:22.49 -03:24:13.9: 14.13 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Forced photometry filter REJECTED candidate at 23:21:22.49 -03:24:13.9: ref_mag=14.17 +/- 0.06 new_mean_mag=14.3049 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:27:07.07 -01:17:41.7: 14.21 +/- 0.09 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:46.02 -06:08:43.9: 14.74 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:27:07.07 -01:17:41.7: 14.22 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Forced photometry filter REJECTED candidate at 23:27:07.07 -01:17:41.7: ref_mag=14.22 +/- 0.06 new_mean_mag=14.3596 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:46.02 -06:08:43.9: 14.53 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:12.27 -03:02:20.7: 14.79 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.12
Forced photometry filter REJECTED candidate at 23:32:46.02 -06:08:43.9: ref_mag=14.62 +/- 0.12 new_mean_mag=14.4401 delta=0.18 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:47.97 -01:06:19.4: 14.61 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:47.97 -01:06:19.4: 14.64 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:12.27 -03:02:20.7: 14.67 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:21:23.09 -03:05:04.6: 14.54 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.11
Forced photometry reference-image weighted average: 14.72 +/- 0.12
Forced photometry filter REJECTED candidate at 23:32:12.27 -03:02:20.7: ref_mag=14.72 +/- 0.12 new_mean_mag=14.4859 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:31:47.97 -01:06:19.4: ref_mag=14.63 +/- 0.11 new_mean_mag=14.4668 delta=0.16 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:23:59.10 +00:39:25.3: 14.42 +/- 0.11 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:21:23.09 -03:05:04.6: 14.40 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.09
Forced photometry filter REJECTED candidate at 23:21:23.09 -03:05:04.6: ref_mag=14.46 +/- 0.09 new_mean_mag=14.5404 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:51.93 -05:33:52.5: 15.27 +/- 0.28 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:23:59.10 +00:39:25.3: 14.63 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:07:31.34 -00:25:45.3: 15.94 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.50 +/- 0.08
Forced photometry filter REJECTED candidate at 23:23:59.10 +00:39:25.3: ref_mag=14.50 +/- 0.08 new_mean_mag=14.5451 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:51.93 -05:33:52.5: 15.24 +/- 0.27 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:07:31.34 -00:25:45.3: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:45.60 -00:31:11.7: 14.57 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.25 +/- 0.19
Forced photometry filter REJECTED candidate at 23:32:51.93 -05:33:52.5: ref_mag=15.25 +/- 0.19 new_mean_mag=14.6595 delta=0.59 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:45.60 -00:31:11.7: 14.61 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.09
Forced photometry filter REJECTED candidate at 23:28:45.60 -00:31:11.7: ref_mag=14.59 +/- 0.09 new_mean_mag=14.5757 delta=0.01 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:17:55.64 -01:45:43.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:24.15 -05:55:30.3: 14.45 +/- 0.14 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:40.05 -03:09:10.2: 14.47 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:17:55.64 -01:45:43.5: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:24.15 -05:55:30.3: 14.89 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:40.05 -03:09:10.2: 14.42 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.12
Forced photometry filter REJECTED candidate at 23:34:24.15 -05:55:30.3: ref_mag=14.59 +/- 0.12 new_mean_mag=14.5218 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 14.44 +/- 0.09
Forced photometry filter REJECTED candidate at 23:34:40.05 -03:09:10.2: ref_mag=14.44 +/- 0.09 new_mean_mag=14.4888 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:09.36 +00:54:10.7: 15.07 +/- 0.20 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:27.21 -04:57:55.6: 14.97 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:03.21 -06:06:08.7: 14.96 +/- 0.23 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:37.94 -05:46:32.8: 14.86 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:27.21 -04:57:55.6: 14.66 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.12
Forced photometry filter REJECTED candidate at 23:26:27.21 -04:57:55.6: ref_mag=14.78 +/- 0.12 new_mean_mag=14.6450 delta=0.13 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:09.36 +00:54:10.7: 14.98 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.14
Forced photometry filter REJECTED candidate at 23:32:09.36 +00:54:10.7: ref_mag=15.02 +/- 0.14 new_mean_mag=14.7169 delta=0.30 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:03.21 -06:06:08.7: 15.23 +/- 0.29 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:37.94 -05:46:32.8: 15.40 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.18
Forced photometry filter REJECTED candidate at 23:32:03.21 -06:06:08.7: ref_mag=15.07 +/- 0.18 new_mean_mag=14.7321 delta=0.34 (need > 0.90)
Forced photometry reference-image weighted average: 15.00 +/- 0.18
Forced photometry filter REJECTED candidate at 23:35:37.94 -05:46:32.8: ref_mag=15.00 +/- 0.18 new_mean_mag=14.7557 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:37.08 +00:27:45.9: 14.96 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:27:15.67 +00:36:03.6: 15.22 +/- 0.22 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:32.44 -01:44:27.4: 14.65 +/- 0.14 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:49.56 -02:55:25.3: 14.92 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:37.08 +00:27:45.9: 15.15 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.15
Forced photometry filter REJECTED candidate at 23:30:37.08 +00:27:45.9: ref_mag=15.04 +/- 0.15 new_mean_mag=14.7782 delta=0.26 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:27:15.67 +00:36:03.6: 15.04 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.15
Forced photometry filter REJECTED candidate at 23:27:15.67 +00:36:03.6: ref_mag=15.12 +/- 0.15 new_mean_mag=14.7623 delta=0.36 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:32.44 -01:44:27.4: 14.80 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:52.04 -02:12:50.1: 14.88 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.10
Forced photometry filter REJECTED candidate at 23:32:32.44 -01:44:27.4: ref_mag=14.72 +/- 0.10 new_mean_mag=14.6265 delta=0.09 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:12.05 -03:17:10.3: 14.76 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:22.76 -04:32:39.0: 14.86 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:49.56 -02:55:25.3: 15.06 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.14
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:35.00 -01:39:03.0: 15.18 +/- 0.25 detection
Forced photometry filter REJECTED candidate at 23:30:49.56 -02:55:25.3: ref_mag=14.98 +/- 0.14 new_mean_mag=14.8200 delta=0.16 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:52.04 -02:12:50.1: 15.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.13
Forced photometry filter REJECTED candidate at 23:32:52.04 -02:12:50.1: ref_mag=14.94 +/- 0.13 new_mean_mag=14.7674 delta=0.17 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:12.05 -03:17:10.3: 15.07 +/- 0.22 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:22.76 -04:32:39.0: 14.90 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.13
Forced photometry filter REJECTED candidate at 23:34:12.05 -03:17:10.3: ref_mag=14.87 +/- 0.13 new_mean_mag=14.6344 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 14.88 +/- 0.13
Forced photometry filter REJECTED candidate at 23:31:22.76 -04:32:39.0: ref_mag=14.88 +/- 0.13 new_mean_mag=14.6920 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:35.00 -01:39:03.0: 14.99 +/- 0.20 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:24.15 -06:03:52.2: 14.98 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:52.90 -06:10:36.5: 14.81 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.16
Forced photometry filter REJECTED candidate at 23:35:35.00 -01:39:03.0: ref_mag=15.07 +/- 0.16 new_mean_mag=14.7170 delta=0.35 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:27.04 -04:33:18.3: 14.98 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:30.49 -03:53:45.3: 15.10 +/- 0.22 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:24.15 -06:03:52.2: 15.07 +/- 0.23 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:52.90 -06:10:36.5: 15.39 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.16
Forced photometry filter REJECTED candidate at 23:30:24.15 -06:03:52.2: ref_mag=15.02 +/- 0.16 new_mean_mag=14.8267 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 14.96 +/- 0.17
Forced photometry filter REJECTED candidate at 23:34:52.90 -06:10:36.5: ref_mag=14.96 +/- 0.17 new_mean_mag=14.7035 delta=0.26 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:27.04 -04:33:18.3: 15.15 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.16
Forced photometry filter REJECTED candidate at 23:34:27.04 -04:33:18.3: ref_mag=15.05 +/- 0.16 new_mean_mag=14.7526 delta=0.30 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:30.49 -03:53:45.3: 14.96 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:05.07 -04:58:08.5: 15.00 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.14
Forced photometry filter REJECTED candidate at 23:28:30.49 -03:53:45.3: ref_mag=15.02 +/- 0.14 new_mean_mag=14.8612 delta=0.16 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:12.55 -03:42:37.4: 15.06 +/- 0.22 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:21.67 -01:06:22.4: 14.84 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:04.11 -05:12:20.3: 15.12 +/- 0.25 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:31:40.97 -04:08:13.3: 14.91 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:05.07 -04:58:08.5: 14.86 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.14
Forced photometry filter REJECTED candidate at 23:32:05.07 -04:58:08.5: ref_mag=14.92 +/- 0.14 new_mean_mag=14.6934 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:12.55 -03:42:37.4: 15.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.15
Forced photometry filter REJECTED candidate at 23:32:12.55 -03:42:37.4: ref_mag=15.04 +/- 0.15 new_mean_mag=14.7827 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:04.11 -05:12:20.3: 15.35 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.19
Forced photometry filter REJECTED candidate at 23:31:04.11 -05:12:20.3: ref_mag=15.21 +/- 0.19 new_mean_mag=14.8656 delta=0.35 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:21.67 -01:06:22.4: 14.85 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.12
Forced photometry filter REJECTED candidate at 23:34:21.67 -01:06:22.4: ref_mag=14.85 +/- 0.12 new_mean_mag=14.7046 delta=0.14 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:27:15.32 -02:46:41.3: 14.84 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:35.15 -03:11:24.0: 15.31 +/- 0.27 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:31:40.97 -04:08:13.3: 15.16 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.15
Forced photometry filter REJECTED candidate at 23:31:40.97 -04:08:13.3: ref_mag=15.01 +/- 0.15 new_mean_mag=14.8625 delta=0.15 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:02.52 -05:01:26.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:20.97 -00:53:20.8: 15.17 +/- 0.20 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:13:08.33 -05:49:59.8: 14.93 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:35.15 -03:11:24.0: 15.06 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.16
Forced photometry filter REJECTED candidate at 23:30:35.15 -03:11:24.0: ref_mag=15.15 +/- 0.16 new_mean_mag=14.8554 delta=0.29 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:27:15.32 -02:46:41.3: 15.47 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.14
Forced photometry filter REJECTED candidate at 23:27:15.32 -02:46:41.3: ref_mag=14.99 +/- 0.14 new_mean_mag=14.8270 delta=0.17 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:02.52 -05:01:26.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:20.97 -00:53:20.8: 15.14 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.14
Forced photometry filter REJECTED candidate at 23:26:20.97 -00:53:20.8: ref_mag=15.16 +/- 0.14 new_mean_mag=14.8572 delta=0.30 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:13:08.33 -05:49:59.8: 15.29 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.14
Forced photometry filter REJECTED candidate at 23:13:08.33 -05:49:59.8: ref_mag=15.06 +/- 0.14 new_mean_mag=14.8367 delta=0.22 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out53009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52874.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
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: 8s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52518_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52518_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52525_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52525_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52526_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52526_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52528_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52528_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52533_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52533_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52534_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52534_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52536_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52536_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52537_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52537_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52540_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52540_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52542_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52542_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52543_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52543_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52553_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52553_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
**** FOUND 23:06:33.79 -03:40:10.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52567_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52567_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52573_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52573_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52604_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52604_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52608_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52608_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52654_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52654_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52655_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52655_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52669_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52669_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52673_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52673_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52740_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52740_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52773_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52773_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52784_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52784_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52791_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52791_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52795_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52795_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52803_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52803_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52812_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52812_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52816_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52816_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52822_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52822_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52828_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52828_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52834_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52834_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52841_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52841_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52858_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52858_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52866_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52866_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52869_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52869_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52874_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
Preparing report for the candidate 52874_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52879_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52879_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52881_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52881_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52886_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52886_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52890_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52890_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52891_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52891_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52895_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52895_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52897_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52897_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52899_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52899_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52901_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52901_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52902_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52902_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52903_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52903_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52911_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52911_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52915_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52915_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52918_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52918_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52923_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52923_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52926_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52926_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52950_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52950_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52954_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52954_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52961_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52961_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52963_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52963_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52967_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52967_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52978_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52978_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52985_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52985_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52993_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52993_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52994_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 52994_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53009_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 53009_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
**** FOUND 23:26:02.52 -05:01:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 1.935 2632909308585212544 351.51004546591 -05.02384921736 14.9224 14.3719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53011_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 53011_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53061_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 53061_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53158_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267
The candidate 53158_fd_Psc-09-Q2b1x1_2026-10-06_00-45-38_20.00sec_-0.00C_LIGHT_0267 did not pass the final checks