This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5
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 11 03.1722 2461347.6722 11.94 23:05:52.26 -05:53:38.0
68.39097 -57.12311 galactic Aqr Second-epoch detections are separated by 0.1" and 11.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.236 Honoria -1 -0 1 12.0 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:05:52.26 -05:53:38.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:05:52.26 -05:53:38.0: 15.60 +/- 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,2461347.6722,11.94,0.05,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 20261103.1722 11.94CV 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 11 03.1722 2461347.6722 13.08 22:54:43.18 +01:20:28.2
73.60465 -50.01027 galactic Psc Second-epoch detections are separated by 0.4" and 11.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.338 Budrosa -1 -0 1 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 22:54:43.18 +01:20:28.2: 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 22:54:43.18 +01:20:28.2: 15.92 +/- 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,2461347.6722,13.08,0.05,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 20261103.1722 13.08CV 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 11 03.1722 2461347.6722 13.37 23:23:55.66 -05:48:20.2
74.68834 -60.20184 galactic Aqr Second-epoch detections are separated by 0.7" and 11.5 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 13.1 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:23:55.66 -05:48:20.2: 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 23:23:55.66 -05:48:20.2: 15.70 +/- 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,2461347.6722,13.37,0.05,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 20261103.1722 13.37CV 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 11 03.1722 2461347.6722 13.87 23:12:25.13 -03:26:15.1
73.66756 -56.52144 galactic Aqr Second-epoch detections are separated by 0.6" and 11.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.570 Kythera -1 -1 1 14.0 0 0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:12:25.13 -03:26:15.1: 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 23:12:25.13 -03:26:15.1: 15.87 +/- 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,2461347.6722,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.1722 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.1722 2461347.6722 13.94 23:06:26.30 -01:43:40.4
73.75715 -54.25186 galactic Psc Second-epoch detections are separated by 1.1" and 11.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.328 Gudrun -1 -0 1 14.2 0 0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:06:26.30 -01:43:40.4: 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 23:06:26.30 -01:43:40.4: 15.93 +/- 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,2461347.6722,13.94,0.05,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 20261103.1722 13.94CV 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 11 03.1722 2461347.6722 14.12 23:08:34.52 -06:10:22.0
68.87277 -57.80331 galactic Aqr Second-epoch detections are separated by 0.6" and 11.3 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 -1 1 14.4 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:08:34.52 -06:10:22.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:08:34.52 -06:10:22.0: 15.75 +/- 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,2461347.6722,14.12,0.05,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 20261103.1722 14.12CV 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 11 03.1722 2461347.6722 14.81 22:58:53.84 -00:44:54.0
72.55907 -52.25224 galactic Psc Second-epoch detections are separated by 1.6" and 11.1 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 0 0 15.1 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 22:58:53.84 -00:44:54.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:58:53.84 -00:44:54.0: 15.94 +/- 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,2461347.6722,14.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.1722 14.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.1722 2461347.6722 14.51 23:12:02.69 +00:53:25.6
78.43108 -53.16952 galactic Psc Second-epoch detections are separated by 1.3" and 11.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1353 Maartje -0 0 0 14.8 -0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:12:02.69 +00:53:25.6: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:12:02.69 +00:53:25.6: 15.92 +/- 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,2461347.6722,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.1722 14.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.1722 2461347.6722 14.81 23:26:14.97 -05:30:26.9
75.96041 -60.35953 galactic Aqr Second-epoch detections are separated by 1.6" and 11.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.223 Rosa -3 1 3 15.1 0 -0
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:14.97 -05:30:26.9: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:14.97 -05:30:26.9: 15.66 +/- 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,2461347.6722,14.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.1722 14.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461347.67243847 03.11.2026 04:08:08.684 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 4919
Objects passed selection criteria: 4914
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 4778
Average stars matched: 4645.75 (97.2321 %)
Memory usage VmPeak: 231884 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Nov 2 23:08:25 CST 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: 2461347.67243847 03.11.2026 04:08:08.684 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
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: 159 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): 28985
Objects passed selection criteria: 28896
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 28356.8
Average stars matched: 26953 (95.0497 %)
Memory usage VmPeak: 253764 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Nov 2 23:12:58 CST 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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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: 2461347.67186601
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits (1st new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Image size: 937.2'x624.1' 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: 23:08:34.408 -01:59:46.99 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 23:08:34.408 -01:59:46.99
Angular distance between the image centers 0.0114 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits (2nd new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
Image size: 937.2'x624.1' 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: 23:08:31.557 -01:58:55.23 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 23:08:31.557 -01:58:55.23
Angular distance between the image centers 0.0287 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 23:08:34.408 -01:59:46.99
Second-epoch second image center 23:08:31.557 -01:58:55.23
Angular distance between the image centers 0.01865 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.iVbn9VUiZC
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.7Cf8QYuAQE
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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits &> /tmp/tmp.bmvNftI9WW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits &> /tmp/tmp.G7wxB6Sal1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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 5 candidate transients before the final filtering. (Hard limit: 10000)
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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
2.3 pix fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
15.4 mag. fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.iVbn9VUiZC (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/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
WCS_HEADER_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits selection=current_pairs N_selected=4338 N_valid=4338 bias_ra_arcsec=-0.006 bias_dec_arcsec=0.002 median_sep_arcsec=0.252 p95_sep_arcsec=0.845 n_q1=1429 n_q2=758 n_q3=1353 n_q4=798 occupied_cells_4x4=16/16
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.7Cf8QYuAQE (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/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=0.381 sigma_q4_arcsec=0.346 n_q1=1416 n_q2=724 n_q3=1303 n_q4=787 worst_quadrant_to_overall_ratio=1.063
WCS_HEADER_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits selection=current_pairs N_selected=4230 N_valid=4230 bias_ra_arcsec=-0.002 bias_dec_arcsec=-0.005 median_sep_arcsec=0.297 p95_sep_arcsec=0.953 n_q1=1416 n_q2=724 n_q3=1303 n_q4=787 occupied_cells_4x4=16/16
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.bmvNftI9WW (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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=1706, passed=6639
Got 6639 stars (including 4617 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat
util/solve_plate_with_UCAC5 got 6639 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 4483 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4475 matched stars entering correct_measured_positions(), 4475 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4475 matched stars entering correct_measured_positions(), 5240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4484 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4477 matched stars entering correct_measured_positions(), 5240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4477 matched stars entering correct_measured_positions(), 5240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4477 stars left (next iteration limit 4922)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4477 robust_rms=7.680 arcsec worst_region_rms=13.689 arcsec outer_annulus_rms=13.689 arcsec
SIP_REFIT: SIP order 3 trial: matched=4477 robust_rms=0.618 arcsec worst_region_rms=0.786 arcsec outer_annulus_rms=0.786 arcsec
SIP_REFIT: SIP order 5 trial: matched=4477 robust_rms=0.329 arcsec worst_region_rms=0.408 arcsec outer_annulus_rms=0.408 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4477 robust_rms_before=1.112 arcsec robust_rms_before_corrected=0.311 arcsec robust_rms_after=0.329 arcsec worst_region_rms_before=0.358 worst_region_rms_after=0.408 outer_annulus_rms_before=1.261 outer_annulus_rms_after=0.408
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.358 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits worst_region_rms_kept=0.358 arcsec robust_rms_kept=0.311 arcsec matched=4477
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits N_match=4477 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.316 n_q1=1484 n_q2=797 n_q3=1370 n_q4=826 worst_quadrant_to_overall_ratio=1.061
WCS_HEADER_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits selection=current_pairs N_selected=4477 N_valid=4477 bias_ra_arcsec=-0.564 bias_dec_arcsec=0.585 median_sep_arcsec=0.980 p95_sep_arcsec=2.124 n_q1=1484 n_q2=797 n_q3=1370 n_q4=826 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits -region wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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.G7wxB6Sal1 (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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=377, bad_region=1706, passed=6602
Got 6602 stars (including 4588 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat
util/solve_plate_with_UCAC5 got 6602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 4454 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4446 matched stars entering correct_measured_positions(), 4446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4446 matched stars entering correct_measured_positions(), 5203 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4455 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4446 matched stars entering correct_measured_positions(), 5203 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4446 matched stars entering correct_measured_positions(), 5203 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4446 stars left (next iteration limit 4890)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4446 robust_rms=7.684 arcsec worst_region_rms=14.316 arcsec outer_annulus_rms=14.316 arcsec
SIP_REFIT: SIP order 3 trial: matched=4446 robust_rms=0.610 arcsec worst_region_rms=0.863 arcsec outer_annulus_rms=0.863 arcsec
SIP_REFIT: SIP order 5 trial: matched=4446 robust_rms=0.323 arcsec worst_region_rms=0.422 arcsec outer_annulus_rms=0.422 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4446 robust_rms_before=1.137 arcsec robust_rms_before_corrected=0.314 arcsec robust_rms_after=0.323 arcsec worst_region_rms_before=0.388 worst_region_rms_after=0.422 outer_annulus_rms_before=1.252 outer_annulus_rms_after=0.422
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.388 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits worst_region_rms_kept=0.388 arcsec robust_rms_kept=0.314 arcsec matched=4446
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits N_match=4446 sigma_overall_arcsec=0.328 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.334 sigma_q3_arcsec=0.333 sigma_q4_arcsec=0.314 n_q1=1486 n_q2=792 n_q3=1360 n_q4=808 worst_quadrant_to_overall_ratio=1.019
WCS_HEADER_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits selection=current_pairs N_selected=4446 N_valid=4446 bias_ra_arcsec=-0.578 bias_dec_arcsec=0.571 median_sep_arcsec=0.985 p95_sep_arcsec=2.168 n_q1=1486 n_q2=792 n_q3=1360 n_q4=808 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits -region wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits to local_wcs_cache/
'wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits' -> 'local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits'
Saving the final (post-refit) wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits to local_wcs_cache/
'wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits' -> 'local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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=1.063
new1=fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits sigma_overall=0.324 worst_q_ratio=1.061
new2=fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits sigma_overall=0.328 worst_q_ratio=1.019
reference average sigma_overall=0.3465 worst_q_ratio=1.0515
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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216_astrometric_residuals.png (4477 matched stars from wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217_astrometric_residuals.png (4446 matched stars from wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits'
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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 -03:04:03.3: 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 23:07:28.80 -02:29:13.5: 12.14 +/- 0.01 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:05:52.26 -05:53:38.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:01:58.97 +00:24:25.3: 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 23:07:13.48 -01:29:21.5: 12.06 +/- 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 -01:29:21.5: 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 23:01:58.97 +00:24:25.3: 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 23:05:52.26 -05:53:38.0: 15.60 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:07:28.80 -02:29:13.5: 12.20 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 23:07:13.48 -01:29:21.5: ref_mag=12.06 +/- 0.01 new_mean_mag=12.0671 delta=-0.00 (need > 0.90)
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 23:01:58.97 +00:24:25.3: ref_mag=12.00 +/- 0.01 new_mean_mag=11.9853 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.17 +/- 0.01
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 -03:04:03.3: 11.57 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 23:07:28.80 -02:29:13.5: ref_mag=12.17 +/- 0.01 new_mean_mag=12.1782 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Forced photometry filter REJECTED candidate at 23:21:26.74 -03:04:03.3: ref_mag=11.57 +/- 0.01 new_mean_mag=11.7351 delta=-0.16 (need > 0.90)
Adding exclusion_list_local.txt__out20218.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 35s
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 20216_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 20216_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20218_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 20218_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20219_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 20219_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20220_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 20220_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20223_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 20223_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 36s
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 ####
23:05:52.26 -05:53:38.0
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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits exists and is non-empty
wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits (1st new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Image size: 937.2'x624.1' 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: 23:08:34.408 -01:59:46.99 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 23:08:34.408 -01:59:46.99
Angular distance between the image centers 0.0114 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits (2nd new image)
verification OK: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
Image size: 937.2'x624.1' 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: 23:08:31.557 -01:58:55.23 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 23:08:31.557 -01:58:55.23
Angular distance between the image centers 0.0287 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 23:08:34.408 -01:59:46.99
Second-epoch second image center 23:08:31.557 -01:58:55.23
Angular distance between the image centers 0.01865 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.uRMpTGnKXd
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.LyBc8Z8mvX
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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits &> /tmp/tmp.rLRuxlMzBU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits &> /tmp/tmp.vkHdPLcQXd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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 38 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
2.1 pix fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
2.2 pix fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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
15.5 mag. fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
15.5 mag. fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.uRMpTGnKXd (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/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=0.318 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
WCS_HEADER_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits selection=current_pairs N_selected=4852 N_valid=4852 bias_ra_arcsec=-0.018 bias_dec_arcsec=0.004 median_sep_arcsec=0.253 p95_sep_arcsec=0.814 n_q1=1558 n_q2=904 n_q3=1485 n_q4=905 occupied_cells_4x4=16/16
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.LyBc8Z8mvX (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/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
WCS_HEADER_DIAG: file=Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits selection=current_pairs N_selected=4854 N_valid=4854 bias_ra_arcsec=-0.023 bias_dec_arcsec=0.002 median_sep_arcsec=0.299 p95_sep_arcsec=0.921 n_q1=1577 n_q2=898 n_q3=1478 n_q4=901 occupied_cells_4x4=16/16
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.rLRuxlMzBU (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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=16, blended=1535, bad_region=7637, passed=36574
Got 36574 stars (including 27717 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat
util/solve_plate_with_UCAC5 got 36574 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 4832 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 30644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4832 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4826 matched stars entering correct_measured_positions(), 30644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4826 matched stars entering correct_measured_positions(), 30644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4826 stars left (next iteration limit 5307)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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=4826 robust_rms=7.469 arcsec worst_region_rms=14.914 arcsec outer_annulus_rms=14.914 arcsec
SIP_REFIT: SIP order 3 trial: matched=4826 robust_rms=0.606 arcsec worst_region_rms=0.862 arcsec outer_annulus_rms=0.862 arcsec
SIP_REFIT: SIP order 5 trial: matched=4826 robust_rms=0.328 arcsec worst_region_rms=0.419 arcsec outer_annulus_rms=0.419 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4826 robust_rms_before=1.123 arcsec robust_rms_before_corrected=0.310 arcsec robust_rms_after=0.328 arcsec worst_region_rms_before=0.376 worst_region_rms_after=0.419 outer_annulus_rms_before=1.293 outer_annulus_rms_after=0.419
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.376 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits worst_region_rms_kept=0.376 arcsec robust_rms_kept=0.310 arcsec matched=4826
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits N_match=4826 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.327 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.318 n_q1=1578 n_q2=900 n_q3=1453 n_q4=895 worst_quadrant_to_overall_ratio=1.026
WCS_HEADER_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits selection=current_pairs N_selected=4826 N_valid=4826 bias_ra_arcsec=-0.586 bias_dec_arcsec=0.586 median_sep_arcsec=0.982 p95_sep_arcsec=2.119 n_q1=1578 n_q2=900 n_q3=1453 n_q4=895 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits -region wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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.vkHdPLcQXd (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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
Checking if the catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS catalog name: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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=13, blended=1495, bad_region=7702, passed=36733
Got 36733 stars (including 27832 good ones) from the SExtractor catalog wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat
util/solve_plate_with_UCAC5 got 36733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 4823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 30722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 30722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 30722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4823 stars left (next iteration limit 5305)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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=4823 robust_rms=7.498 arcsec worst_region_rms=14.356 arcsec outer_annulus_rms=14.356 arcsec
SIP_REFIT: SIP order 3 trial: matched=4823 robust_rms=0.585 arcsec worst_region_rms=1.031 arcsec outer_annulus_rms=1.031 arcsec
SIP_REFIT: SIP order 5 trial: matched=4823 robust_rms=0.319 arcsec worst_region_rms=0.430 arcsec outer_annulus_rms=0.430 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4823 robust_rms_before=1.155 arcsec robust_rms_before_corrected=0.303 arcsec robust_rms_after=0.319 arcsec worst_region_rms_before=0.372 worst_region_rms_after=0.430 outer_annulus_rms_before=1.266 outer_annulus_rms_after=0.430
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.372 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits worst_region_rms_kept=0.372 arcsec robust_rms_kept=0.303 arcsec matched=4823
WCS_QUALITY_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits N_match=4823 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.335 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.301 n_q1=1583 n_q2=892 n_q3=1454 n_q4=894 worst_quadrant_to_overall_ratio=1.046
WCS_HEADER_DIAG: file=fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits selection=current_pairs N_selected=4823 N_valid=4823 bias_ra_arcsec=-0.596 bias_dec_arcsec=0.572 median_sep_arcsec=0.990 p95_sep_arcsec=2.149 n_q1=1583 n_q2=892 n_q3=1454 n_q4=894 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits -region wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-07-19_20.00sec_-0.00C_LIGHT_0216.fits
Saving fully-calibrated image wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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_2026-11-02_CI_Psc-09-Q2b1x1_221502_TTUQ2b1x1_3201448_PP6v3BB5/wcs_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217.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 22:54:43.18 +01:20:28.2: 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 23:13:05.87 -01:08:42.9: 14.55 +/- 0.11 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:23:55.66 -05:48:20.2: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 22:57:22.16 -06:11:43.6: 14.52 +/- 0.12 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:12:25.13 -03:26:15.1: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:24.17 -05:55:30.9: 14.46 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:08:34.52 -06:10:22.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:06:26.30 -01:43:40.4: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:06.37 +00:02:55.6: 13.99 +/- 0.08 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:57:22.16 -06:11:43.6: 14.38 +/- 0.11 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:06.37 +00:02:55.6: 13.99 +/- 0.08 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:23:55.66 -05:48:20.2: 15.70 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Forced photometry filter REJECTED candidate at 23:32:06.37 +00:02:55.6: ref_mag=13.99 +/- 0.05 new_mean_mag=14.1282 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 23:08:34.52 -06:10:22.0: 15.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.44 +/- 0.08
Forced photometry filter REJECTED candidate at 22:57:22.16 -06:11:43.6: ref_mag=14.44 +/- 0.08 new_mean_mag=14.3730 delta=0.07 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:14:34.29 +02:10:31.6: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:12:25.13 -03:26:15.1: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:24.17 -05:55:30.9: 14.91 +/- 0.22 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:54:43.18 +01:20:28.2: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:13:05.87 -01:08:42.9: 14.63 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.12
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:06:26.30 -01:43:40.4: 15.93 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:34:24.17 -05:55:30.9: ref_mag=14.60 +/- 0.12 new_mean_mag=14.4311 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 14.59 +/- 0.08
Forced photometry filter REJECTED candidate at 23:13:05.87 -01:08:42.9: ref_mag=14.59 +/- 0.08 new_mean_mag=14.5514 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:14:34.29 +02:10:31.6: 14.67 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter REJECTED candidate at 23:14:34.29 +02:10:31.6: ref_mag=13.74 +/- 0.04 new_mean_mag=14.5150 delta=-0.78 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:33:16.11 -02:10:46.9: 14.87 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:43.70 -02:57:43.4: 14.77 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:27.23 -05:01:24.0: 14.88 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:27.24 -04:57:56.9: 15.02 +/- 0.20 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:33:16.11 -02:10:46.9: 14.51 +/- 0.13 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:43.70 -02:57:43.4: 14.75 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:27.23 -05:01:24.0: 15.17 +/- 0.23 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:27.24 -04:57:56.9: 14.70 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:08:48.90 -03:10:33.8: 14.52 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.12
Forced photometry filter REJECTED candidate at 23:26:27.24 -04:57:56.9: ref_mag=14.82 +/- 0.12 new_mean_mag=14.6746 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 14.76 +/- 0.12
Forced photometry reference-image weighted average: 14.99 +/- 0.14
Forced photometry filter REJECTED candidate at 23:35:43.70 -02:57:43.4: ref_mag=14.76 +/- 0.12 new_mean_mag=14.4604 delta=0.30 (need > 0.90)
Forced photometry reference-image weighted average: 14.63 +/- 0.10
Forced photometry filter REJECTED candidate at 23:26:27.23 -05:01:24.0: ref_mag=14.99 +/- 0.14 new_mean_mag=14.7121 delta=0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:33:16.11 -02:10:46.9: ref_mag=14.63 +/- 0.10 new_mean_mag=14.5601 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 23:08:48.90 -03:10:33.8: 14.95 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.09
Forced photometry filter REJECTED candidate at 23:08:48.90 -03:10:33.8: ref_mag=14.65 +/- 0.09 new_mean_mag=14.7097 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 22:58:53.84 -00:44:54.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:33:03.28 +01:24:27.7: 15.05 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:46.00 -06:08:43.9: 14.74 +/- 0.19 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:12:02.69 +00:53:25.6: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:58:53.84 -00:44:54.0: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:23:48.49 -06:03:37.4: 15.00 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:46.00 -06:08:43.9: 14.54 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:33:03.28 +01:24:27.7: 15.45 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.12
Forced photometry reference-image weighted average: 15.19 +/- 0.17
Forced photometry filter REJECTED candidate at 23:32:46.00 -06:08:43.9: ref_mag=14.62 +/- 0.12 new_mean_mag=14.5201 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:33:03.28 +01:24:27.7: ref_mag=15.19 +/- 0.17 new_mean_mag=14.7863 delta=0.40 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:12:02.69 +00:53:25.6: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:23:48.49 -06:03:37.4: 14.94 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.14
Forced photometry filter REJECTED candidate at 23:23:48.49 -06:03:37.4: ref_mag=14.97 +/- 0.14 new_mean_mag=14.7844 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 22:54:12.27 -05:28:27.1: 14.71 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:25:01.74 -06:04:51.6: 14.79 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:36.69 -01:58:55.9: 14.61 +/- 0.14 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:25:01.74 -06:04:51.6: 14.56 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.10
Forced photometry filter REJECTED candidate at 23:25:01.74 -06:04:51.6: ref_mag=14.65 +/- 0.10 new_mean_mag=14.7610 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:36.69 -01:58:55.9: 14.78 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Forced photometry filter REJECTED candidate at 23:34:36.69 -01:58:55.9: ref_mag=14.69 +/- 0.11 new_mean_mag=14.7593 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 22:54:12.27 -05:28:27.1: 15.13 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.13
Forced photometry filter REJECTED candidate at 22:54:12.27 -05:28:27.1: ref_mag=14.84 +/- 0.13 new_mean_mag=14.6658 delta=0.17 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 22:58:38.36 -03:01:27.3: 15.49 +/- 0.26 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:35.07 -01:39:03.6: 15.16 +/- 0.24 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:20:34.51 -05:30:05.2: 14.90 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:58:38.36 -03:01:27.3: 14.82 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.12
Forced photometry filter REJECTED candidate at 22:58:38.36 -03:01:27.3: ref_mag=14.97 +/- 0.12 new_mean_mag=14.8142 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 23:35:35.07 -01:39:03.6: 15.00 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:20:34.51 -05:30:05.2: 14.66 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.16
Forced photometry reference-image weighted average: 14.75 +/- 0.11
Forced photometry filter REJECTED candidate at 23:35:35.07 -01:39:03.6: ref_mag=15.07 +/- 0.16 new_mean_mag=14.5005 delta=0.57 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:20:34.51 -05:30:05.2: ref_mag=14.75 +/- 0.11 new_mean_mag=14.6611 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 23:32:00.52 +01:18:37.1: 15.11 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:50.65 +00:02:19.4: 15.09 +/- 0.23 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:32:27.96 +00:59:44.1: 14.70 +/- 0.16 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:50.65 +00:02:19.4: 14.97 +/- 0.20 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:00.52 +01:18:37.1: 15.08 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.15
Forced photometry filter REJECTED candidate at 23:34:50.65 +00:02:19.4: ref_mag=15.02 +/- 0.15 new_mean_mag=14.8042 delta=0.22 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:32:27.96 +00:59:44.1: 14.65 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.15
Forced photometry reference-image weighted average: 14.67 +/- 0.11
Forced photometry filter REJECTED candidate at 23:32:00.52 +01:18:37.1: ref_mag=15.10 +/- 0.15 new_mean_mag=14.6662 delta=0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:32:27.96 +00:59:44.1: ref_mag=14.67 +/- 0.11 new_mean_mag=14.7061 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:30:00.59 +00:44:33.9: 15.13 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:34:21.71 -01:06:22.5: 14.86 +/- 0.17 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:36:05.34 -03:08:48.7: 14.97 +/- 0.21 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:30:00.59 +00:44:33.9: 14.89 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.13
Forced photometry filter REJECTED candidate at 23:30:00.59 +00:44:33.9: ref_mag=14.98 +/- 0.13 new_mean_mag=14.7938 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 23:34:21.71 -01:06:22.5: 14.88 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:36:05.34 -03:08:48.7: 14.60 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 23:34:21.71 -01:06:22.5: ref_mag=14.87 +/- 0.12 new_mean_mag=14.6420 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 14.71 +/- 0.12
Forced photometry filter REJECTED candidate at 23:36:05.34 -03:08:48.7: ref_mag=14.71 +/- 0.12 new_mean_mag=14.7135 delta=0.00 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:35:55.95 +00:18:37.5: 14.64 +/- 0.15 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:35:55.95 +00:18:37.5: 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 22:51:02.48 -03:13:00.0: 15.59 +/- 0.29 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:28:30.54 -03:53:46.1: 15.05 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.11
Forced photometry filter REJECTED candidate at 23:35:55.95 +00:18:37.5: ref_mag=14.71 +/- 0.11 new_mean_mag=14.8057 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 22:51:02.48 -03:13:00.0: 15.20 +/- 0.20 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:28:30.54 -03:53:46.1: 14.97 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.17
Forced photometry reference-image weighted average: 15.01 +/- 0.14
Forced photometry filter REJECTED candidate at 22:51:02.48 -03:13:00.0: ref_mag=15.33 +/- 0.17 new_mean_mag=14.8722 delta=0.46 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:28:30.54 -03:53:46.1: ref_mag=15.01 +/- 0.14 new_mean_mag=14.9010 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 23:34:10.08 -02:20:24.1: 14.87 +/- 0.18 detection
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:34:10.08 -02:20:24.1: 15.00 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.13
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-27-09_20.00sec_4.90C_LIGHT_1017.fits at 23:26:14.97 -05:30:26.9: 15.65 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:34:10.08 -02:20:24.1: ref_mag=14.93 +/- 0.13 new_mean_mag=14.8291 delta=0.10 (need > 0.90)
Forced photometry on wcs_Psc-09-Q2b1x1_2026-07-21_05-28-24_20.00sec_4.90C_LIGHT_1018.fits at 23:26:14.97 -05:30:26.9: 15.66 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out52626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53053.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 44s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 52521_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52521_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52525_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52525_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52551_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52551_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 23:05:52.25 -05:53:37.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52626_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 52626_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 52666_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 52666_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 52746_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 52746_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 52791_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 52791_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 52816_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 52816_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 52819_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52819_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52887_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52887_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52908_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52908_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52912_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52912_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52920_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52920_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52928_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52928_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52931_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52931_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52935_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52935_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52937_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 52937_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 52957_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 52957_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 52958_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52958_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52972_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52972_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52977_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52977_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52982_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52982_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52987_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52987_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52989_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52989_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52990_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52990_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52993_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52993_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 52998_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 52998_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53001_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53001_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53006_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53006_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53010_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53010_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53012_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53012_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53020_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53020_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53027_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53027_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53045_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53045_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53049_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53049_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53050_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53050_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 53051_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217
The candidate 53051_fd_Psc-09-Q2b1x1_2026-11-02_22-08-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
