This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 12.50 01:45:53.39 +10:30:56.6
144.08185 -50.10662 galactic Psc Second-epoch detections are separated by 1.0" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.124 Alkeste -0 0 0 12.5 -0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:53.39 +10:30:56.6: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:53.39 +10:30:56.6: 16.05 +/- 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,2461289.9502,12.50,0.05,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 20260906.4502 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 12.98 01:42:15.11 +16:11:15.4
140.29797 -44.96387 galactic Psc Second-epoch detections are separated by 1.7" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.212 Medea -0 0 0 13.2 -0 -0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:15.11 +16:11:15.4: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:42:15.11 +16:11:15.4: 16.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.9502,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260906.4502 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 13.75 01:55:11.89 +10:11:48.2
147.57954 -49.59920 galactic Psc Second-epoch detections are separated by 0.8" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.167 Urda -0 -0 0 14.0 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:55:11.89 +10:11:48.2: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:55:11.89 +10:11:48.2: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.9502,13.75,0.05,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 20260906.4502 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 13.70 01:54:24.12 +13:51:20.1
145.32569 -46.26039 galactic Ari Second-epoch detections are separated by 0.9" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.147 Protogeneia -0 -0 0 13.8 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:24.12 +13:51:20.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:24.12 +13:51:20.1: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.4501* 01 54 24.12 +13 51 20.1 13.7 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.9502,13.70,0.05,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 20260906.4502 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 13.83 01:54:52.87 +15:57:09.0
144.45420 -44.25184 galactic Ari Second-epoch detections are separated by 0.2" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.295 Theresia 0 -0 0 14.0 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:52.87 +15:57:09.0: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:52.87 +15:57:09.0: 16.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.4501* 01 54 52.87 +15 57 09.0 13.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.9502,13.83,0.05,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 20260906.4502 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 14.09 01:46:22.69 +15:01:32.8
142.13109 -45.78790 galactic Psc Second-epoch detections are separated by 1.9" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1317 Silvretta -1 0 1 14.2 -0 -0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:46:22.69 +15:01:32.8: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:46:22.69 +15:01:32.8: 16.16 +/- 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,2461289.9502,14.09,0.05,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 20260906.4502 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 14.22 01:53:50.37 +14:41:37.2
144.72603 -45.52095 galactic Ari Second-epoch detections are separated by 1.1" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1572 Posnania -1 -1 1 14.4 -0 -0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:50.37 +14:41:37.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:50.37 +14:41:37.2: 16.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.4501* 01 53 50.37 +14 41 37.2 14.2 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.9502,14.22,0.05,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 20260906.4502 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 14.59 02:07:54.37 +10:38:07.7
151.64102 -47.92810 galactic Ari Second-epoch detections are separated by 2.3" 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.401 Ottilia -1 0 1 14.8 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:07:54.37 +10:38:07.7: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:07:54.37 +10:38:07.7: 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!
TCP 2026 09 06.4501* 02 07 54.37 +10 38 07.7 14.6 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.9502,14.59,0.05,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 20260906.4502 14.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 14.86 01:58:29.39 +12:25:35.7
147.43698 -47.22974 galactic Ari Second-epoch detections are separated by 4.4" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2675 Tolkien -1 0 1 15.3 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:58:29.39 +12:25:35.7: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:58:29.39 +12:25:35.7: 16.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.4501* 01 58 29.39 +12 25 35.7 14.9 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.9502,14.86,0.05,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 20260906.4502 14.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.4502 2461289.9502 13.82 01:39:29.85 +15:11:59.5
139.77068 -46.09465 galactic Psc Second-epoch detections are separated by 0.6" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.517 Edith -0 -1 1 14.0 -0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:29.85 +15:11:59.5: 16.10 +/- 0.31 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:29.85 +15:11:59.5: 15.93 +/- 0.30 detection
Forced photometry reference-image weighted average: 16.01 +/- 0.21
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,2461289.9502,13.82,0.05,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 20260906.4502 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461289.95046190 06.09.2026 10:48:29.908 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5505
Objects passed selection criteria: 5502
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: 5351.5
Average stars matched: 5301 (99.0563 %)
Memory usage VmPeak: 232824 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 05:52:40 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461289.95046190 06.09.2026 10:48:29.908 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 51
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 15 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): 31624
Objects passed selection criteria: 31536
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 30561
Average stars matched: 29806.5 (97.5312 %)
Memory usage VmPeak: 260312 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 05:53:37 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
SExtractor catalog cache: saved Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461289.94984508
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.869 +14:00:12.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Image size: 937.3'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: 01:46:41.076 +13:59:52.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:41.076 +13:59:52.55
Angular distance between the image centers 0.0073 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Image size: 937.3'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: 01:46:43.667 +14:00:41.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:43.667 +14:00:41.89
Angular distance between the image centers 0.0174 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:46:41.076 +13:59:52.55
Second-epoch second image center 01:46:43.667 +14:00:41.89
Angular distance between the image centers 0.01725 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.1wos8XZjcd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.83Y2nCoTRx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits &> /tmp/tmp.W09Ry93b6G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits &> /tmp/tmp.1Wt30TNgAv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.943700
a=0.000000 b=1.000000 c=22.943700
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=5.9)
Read 6762 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4566 to 34.9567 deg, Dec +8.6053 to +19.2739 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.4566 to 34.9567 deg, Dec 8.6053 to 19.2739 deg
Loaded 4732 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3812 out of 4016 total matches.
Matched with Tycho-2 4016 out of 6762 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.0 pix Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.3 pix fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
2.3 pix fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.3 mag. Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.2 mag. fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
15.2 mag. fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
All-image limiting magnitude estimate: 15.2 (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.1wos8XZjcd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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=549, bad_region=1800, passed=7679
Got 7679 stars (including 5466 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 7679 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 6238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 6238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 6238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4879 stars left (next iteration limit 5366)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4879 sigma_overall_arcsec=0.245 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.220 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.211 n_q1=1608 n_q2=884 n_q3=1498 n_q4=889 worst_quadrant_to_overall_ratio=1.322
The image catalog is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.83Y2nCoTRx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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=519, bad_region=1590, passed=6762
Got 6762 stars (including 4768 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 6762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4664 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 4658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4664 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4658 stars left (next iteration limit 5123)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4658 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.252 n_q1=1483 n_q2=869 n_q3=1437 n_q4=869 worst_quadrant_to_overall_ratio=1.350
The image catalog is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.W09Ry93b6G (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.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=448, bad_region=1587, passed=6851
Got 6851 stars (including 4917 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat
util/solve_plate_with_UCAC5 got 6851 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4806 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 4802 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 5569 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 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4807 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 5569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 5569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4802 stars left (next iteration limit 5282)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4802 robust_rms=6.765 arcsec worst_quadrant_rms=10.303 arcsec
SIP_REFIT: SIP order 3 trial: matched=4802 robust_rms=0.511 arcsec worst_quadrant_rms=0.616 arcsec
SIP_REFIT: SIP order 5 trial: matched=4802 robust_rms=0.327 arcsec worst_quadrant_rms=0.356 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4802 robust_rms_before=1.097 arcsec robust_rms_before_corrected=0.323 arcsec robust_rms_after=0.327 arcsec worst_quadrant_rms_before=0.343 worst_quadrant_rms_after=0.356
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.343 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits N_match=4802 sigma_overall_arcsec=0.338 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.314 n_q1=1605 n_q2=864 n_q3=1488 n_q4=845 worst_quadrant_to_overall_ratio=1.068
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits -region wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.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.1Wt30TNgAv (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.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=459, bad_region=1581, passed=6779
Got 6779 stars (including 4827 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat
util/solve_plate_with_UCAC5 got 6779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4716 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4712 matched stars entering correct_measured_positions(), 4712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4712 matched stars entering correct_measured_positions(), 5497 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4716 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4712 matched stars entering correct_measured_positions(), 5497 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4712 matched stars entering correct_measured_positions(), 5497 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4712 stars left (next iteration limit 5183)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4712 robust_rms=6.760 arcsec worst_quadrant_rms=10.332 arcsec
SIP_REFIT: SIP order 3 trial: matched=4712 robust_rms=0.569 arcsec worst_quadrant_rms=0.659 arcsec
SIP_REFIT: SIP order 5 trial: matched=4712 robust_rms=0.389 arcsec worst_quadrant_rms=0.420 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4712 robust_rms_before=1.129 arcsec robust_rms_before_corrected=0.389 arcsec robust_rms_after=0.389 arcsec worst_quadrant_rms_before=0.415 worst_quadrant_rms_after=0.420
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.415 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits N_match=4712 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.391 sigma_q3_arcsec=0.455 sigma_q4_arcsec=0.379 n_q1=1575 n_q2=842 n_q3=1465 n_q4=830 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits -region wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
Saving the final (post-refit) wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits sigma_overall=0.245 worst_q_ratio=1.322
ref2=Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits sigma_overall=0.312 worst_q_ratio=1.350
new1=fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits sigma_overall=0.338 worst_q_ratio=1.068
new2=fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits sigma_overall=0.407 worst_q_ratio=1.118
reference average sigma_overall=0.2785 worst_q_ratio=1.336
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_astrometric_residuals.png (4879 matched stars from wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.22 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139_astrometric_residuals.png (4658 matched stars from wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452_astrometric_residuals.png (4802 matched stars from wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453_astrometric_residuals.png (4712 matched stars from wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits'
Preparing the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-03-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 ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
SExtractor catalog cache: saved Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Creating symlink local_wcs_cache/wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.869 +14:00:12.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Image size: 937.3'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: 01:46:41.076 +13:59:52.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:41.076 +13:59:52.55
Angular distance between the image centers 0.0073 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Image size: 937.3'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: 01:46:43.667 +14:00:41.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:43.667 +14:00:41.89
Angular distance between the image centers 0.0174 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:46:41.076 +13:59:52.55
Second-epoch second image center 01:46:43.667 +14:00:41.89
Angular distance between the image centers 0.01725 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.3UAziCAgPU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.enlRimNaw7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits &> /tmp/tmp.La68Ez47DN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits &> /tmp/tmp.D5nb4kh5Nl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.837800
a=0.000000 b=1.000000 c=22.837800
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=4.7)
Read 38153 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4016 to 34.9977 deg, Dec +8.5904 to +19.2796 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.4016 to 34.9977 deg, Dec 8.5904 to 19.2796 deg
Loaded 4774 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3712 out of 4109 total matches.
Matched with Tycho-2 4109 out of 38153 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 40 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
1.9 pix Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.2 pix fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
2.1 pix fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Limiting magnitude estimates:
15.6 mag. Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.4 mag. Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.3 mag. fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
15.3 mag. fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.3UAziCAgPU (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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=7, blended=1873, bad_region=7665, passed=40632
Got 40632 stars (including 31385 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 40632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 4884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 34591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 34591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 34591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4884 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4884 sigma_overall_arcsec=0.239 sigma_q1_arcsec=0.309 sigma_q2_arcsec=0.215 sigma_q3_arcsec=0.219 sigma_q4_arcsec=0.202 n_q1=1599 n_q2=913 n_q3=1491 n_q4=881 worst_quadrant_to_overall_ratio=1.292
The image catalog is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.enlRimNaw7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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=1585, bad_region=7065, passed=38140
Got 38140 stars (including 29739 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 38140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 32593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 32593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 32593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4888 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4888 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.414 sigma_q2_arcsec=0.266 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.248 n_q1=1608 n_q2=911 n_q3=1499 n_q4=870 worst_quadrant_to_overall_ratio=1.364
The image catalog is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.La68Ez47DN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.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=1503, bad_region=6961, passed=36126
Got 36126 stars (including 27943 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat
util/solve_plate_with_UCAC5 got 36126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 4876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 30825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 30825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 30825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4876 stars left (next iteration limit 5363)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.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=4876 robust_rms=6.533 arcsec worst_quadrant_rms=9.557 arcsec
SIP_REFIT: SIP order 3 trial: matched=4876 robust_rms=0.494 arcsec worst_quadrant_rms=0.611 arcsec
SIP_REFIT: SIP order 5 trial: matched=4876 robust_rms=0.321 arcsec worst_quadrant_rms=0.347 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4876 robust_rms_before=1.111 arcsec robust_rms_before_corrected=0.319 arcsec robust_rms_after=0.321 arcsec worst_quadrant_rms_before=0.343 worst_quadrant_rms_after=0.347
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.343 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits N_match=4876 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.308 n_q1=1610 n_q2=937 n_q3=1445 n_q4=884 worst_quadrant_to_overall_ratio=1.068
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits -region wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.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.D5nb4kh5Nl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.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=14, blended=1513, bad_region=7061, passed=36746
Got 36746 stars (including 28433 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat
util/solve_plate_with_UCAC5 got 36746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 31335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 31335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 31334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.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=4873 robust_rms=6.566 arcsec worst_quadrant_rms=9.227 arcsec
SIP_REFIT: SIP order 3 trial: matched=4873 robust_rms=0.549 arcsec worst_quadrant_rms=0.634 arcsec
SIP_REFIT: SIP order 5 trial: matched=4873 robust_rms=0.386 arcsec worst_quadrant_rms=0.414 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4873 robust_rms_before=1.135 arcsec robust_rms_before_corrected=0.380 arcsec robust_rms_after=0.386 arcsec worst_quadrant_rms_before=0.405 worst_quadrant_rms_after=0.414
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.405 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits N_match=4873 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.369 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.429 sigma_q4_arcsec=0.365 n_q1=1613 n_q2=931 n_q3=1433 n_q4=896 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits -region wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-47-36_20.00sec_-0.00C_LIGHT_0452.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Psc-03-Q2b1x1_055022_TTUQ2b1x1_2156759_Ei1RgQFx/wcs_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453.fits
Preparing the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:55:11.89 +10:11:48.2: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:05.58 +13:26:18.6: 12.95 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:53.39 +10:30:56.6: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:09:39.78 +13:36:48.6: 12.46 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:17.17 +17:31:16.6: 13.61 +/- 0.04 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:24.12 +13:51:20.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:11.38 +10:40:00.8: 15.07 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:15.11 +16:11:15.4: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:26.69 +12:54:47.0: 14.72 +/- 0.09 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:06:51.97 +09:46:30.9: 14.14 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:17.17 +17:31:16.6: 13.65 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:11.38 +10:40:00.8: 14.87 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:09:39.78 +13:36:48.6: 12.51 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:24.12 +13:51:20.1: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:55:11.89 +10:11:48.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:05.58 +13:26:18.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:42:15.11 +16:11:15.4: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:06:51.97 +09:46:30.9: 14.18 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:26.69 +12:54:47.0: 14.72 +/- 0.10 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:53.39 +10:30:56.6: 16.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry reference-image weighted average: 14.96 +/- 0.10
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry reference-image weighted average: 14.72 +/- 0.07
Forced photometry filter REJECTED candidate at 01:31:17.17 +17:31:16.6: ref_mag=13.63 +/- 0.03 new_mean_mag=14.1149 delta=-0.49 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:31:11.38 +10:40:00.8: ref_mag=14.96 +/- 0.10 new_mean_mag=14.9505 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.16 +/- 0.05
Forced photometry filter REJECTED candidate at 02:09:39.78 +13:36:48.6: ref_mag=12.48 +/- 0.01 new_mean_mag=12.8130 delta=-0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:31:05.58 +13:26:18.6: ref_mag=12.96 +/- 0.02 new_mean_mag=13.0732 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:39:26.69 +12:54:47.0: ref_mag=14.72 +/- 0.07 new_mean_mag=14.8463 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:06:51.97 +09:46:30.9: ref_mag=14.16 +/- 0.05 new_mean_mag=14.3176 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:52.87 +15:57:09.0: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:48:50.91 +16:23:37.0: 13.84 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:50.37 +14:41:37.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:43:42.63 +12:53:22.9: 14.17 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:46:22.69 +15:01:32.8: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:58.38 +14:22:00.7: 14.33 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:52.87 +15:57:09.0: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:48:50.91 +16:23:37.0: 13.81 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:43:42.63 +12:53:22.9: 13.99 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:50.37 +14:41:37.2: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:46:22.69 +15:01:32.8: 16.16 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter REJECTED candidate at 01:48:50.91 +16:23:37.0: ref_mag=13.82 +/- 0.04 new_mean_mag=13.8688 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry filter REJECTED candidate at 01:43:42.63 +12:53:22.9: ref_mag=14.07 +/- 0.04 new_mean_mag=14.0460 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:58.38 +14:22:00.7: 14.40 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.06
Forced photometry filter REJECTED candidate at 01:34:58.38 +14:22:00.7: ref_mag=14.36 +/- 0.06 new_mean_mag=14.5559 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:52.16 +13:46:27.8: 14.65 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:25.10 +16:56:06.6: 14.85 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:07:54.37 +10:38:07.7: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:52.16 +13:46:27.8: 14.88 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.07
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:30:25.10 +16:56:06.6: 14.95 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 01:45:52.16 +13:46:27.8: ref_mag=14.72 +/- 0.07 new_mean_mag=14.7006 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 14.89 +/- 0.10
Forced photometry filter REJECTED candidate at 01:30:25.10 +16:56:06.6: ref_mag=14.89 +/- 0.10 new_mean_mag=14.7340 delta=0.16 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:07:54.37 +10:38:07.7: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:36:20.40 +14:59:58.2: 14.82 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:33:40.50 +10:25:24.0: 15.59 +/- 0.23 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:36:20.40 +14:59:58.2: 14.93 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.09
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:33:40.50 +10:25:24.0: 15.10 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 01:36:20.40 +14:59:58.2: ref_mag=14.87 +/- 0.09 new_mean_mag=14.8523 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 15.27 +/- 0.14
Forced photometry filter REJECTED candidate at 01:33:40.50 +10:25:24.0: ref_mag=15.27 +/- 0.14 new_mean_mag=14.9132 delta=0.36 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:29:45.25 +10:12:41.3: 15.17 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:41.41 +10:14:09.9: 15.18 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:29:45.25 +10:12:41.3: 15.14 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.13
Forced photometry filter REJECTED candidate at 01:29:45.25 +10:12:41.3: ref_mag=15.15 +/- 0.13 new_mean_mag=14.9262 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:30:41.41 +10:14:09.9: 15.09 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.11
Forced photometry filter REJECTED candidate at 01:30:41.41 +10:14:09.9: ref_mag=15.14 +/- 0.11 new_mean_mag=14.9613 delta=0.18 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:42.30 +14:54:33.6: 15.32 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:58:29.39 +12:25:35.7: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:30:42.30 +14:54:33.6: 15.30 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.13
Forced photometry filter REJECTED candidate at 01:30:42.30 +14:54:33.6: ref_mag=15.31 +/- 0.13 new_mean_mag=15.0761 delta=0.24 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:58:29.39 +12:25:35.7: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:02.54 +17:25:06.5: 15.21 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:02.54 +17:25:06.5: 15.26 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.13
Forced photometry filter REJECTED candidate at 01:28:02.54 +17:25:06.5: ref_mag=15.23 +/- 0.13 new_mean_mag=15.1147 delta=0.12 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:15.50 +16:53:34.1: 15.05 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:15.50 +16:53:34.1: 14.88 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.09
Forced photometry filter REJECTED candidate at 01:31:15.50 +16:53:34.1: ref_mag=14.97 +/- 0.09 new_mean_mag=15.0182 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:29:14.83 +10:02:58.3: 15.26 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:29:14.83 +10:02:58.3: 15.05 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.12
Forced photometry filter REJECTED candidate at 01:29:14.83 +10:02:58.3: ref_mag=15.15 +/- 0.12 new_mean_mag=15.0959 delta=0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:32:42.23 +14:15:08.8: 15.15 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:32:42.23 +14:15:08.8: 15.59 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.12
Forced photometry filter REJECTED candidate at 01:32:42.23 +14:15:08.8: ref_mag=15.26 +/- 0.12 new_mean_mag=15.1342 delta=0.12 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:59:33.34 +10:00:38.9: 15.31 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:59:33.34 +10:00:38.9: 15.38 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.34 +/- 0.14
Forced photometry filter REJECTED candidate at 01:59:33.34 +10:00:38.9: ref_mag=15.34 +/- 0.14 new_mean_mag=15.0261 delta=0.32 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:25.02 +14:56:05.6: 15.02 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:39.34 +15:06:44.1: 15.32 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:20.57 +16:57:06.5: 15.54 +/- 0.21 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:56.23 +14:59:32.4: 14.81 +/- 0.09 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:25.02 +14:56:05.6: 15.35 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.11
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:50:39.34 +15:06:44.1: 15.25 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 01:28:25.02 +14:56:05.6: ref_mag=15.12 +/- 0.11 new_mean_mag=15.1096 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 15.28 +/- 0.11
Forced photometry filter REJECTED candidate at 01:50:39.34 +15:06:44.1: ref_mag=15.28 +/- 0.11 new_mean_mag=15.1128 delta=0.17 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:38:20.57 +16:57:06.5: 15.46 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.50 +/- 0.15
Forced photometry filter REJECTED candidate at 01:38:20.57 +16:57:06.5: ref_mag=15.50 +/- 0.15 new_mean_mag=15.0354 delta=0.46 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:50:56.23 +14:59:32.4: 14.76 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.07
Forced photometry filter REJECTED candidate at 01:50:56.23 +14:59:32.4: ref_mag=14.79 +/- 0.07 new_mean_mag=14.8694 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:53.67 +10:13:34.3: 15.48 +/- 0.22 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:54.81 +11:10:49.3: 15.15 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:53.67 +10:13:34.3: 15.24 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.35 +/- 0.15
Forced photometry filter REJECTED candidate at 01:28:53.67 +10:13:34.3: ref_mag=15.35 +/- 0.15 new_mean_mag=15.0393 delta=0.31 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:59:20.82 +10:40:13.7: 15.44 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:29.85 +15:11:59.5: 16.10 +/- 0.31 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:54.81 +11:10:49.3: 15.03 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.11
Forced photometry filter REJECTED candidate at 01:28:54.81 +11:10:49.3: ref_mag=15.09 +/- 0.11 new_mean_mag=15.0759 delta=0.02 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:59:20.82 +10:40:13.7: 15.28 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.13
Forced photometry filter REJECTED candidate at 01:59:20.82 +10:40:13.7: ref_mag=15.36 +/- 0.13 new_mean_mag=15.0091 delta=0.35 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:29.85 +15:11:59.5: 15.93 +/- 0.30 detection
Forced photometry reference-image weighted average: 16.01 +/- 0.21
Forced photometry filter KEPT candidate at 01:39:29.85 +15:11:59.5: ref_mag=16.01 +/- 0.21 new_mean_mag=13.8234 delta=2.19 (need > 0.90)
Adding exclusion_list_local.txt__out16861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51677.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 51441_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51441_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51445_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51445_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51451_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51451_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51460_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51460_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51463_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51463_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51476_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51476_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51484_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51484_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51487_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51487_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51527_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51527_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51529_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51529_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51530_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51530_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
**** FOUND 01:39:44.54 +16:26:02.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 51536_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51536_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51537_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51537_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51556_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51556_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51563_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51563_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51570_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51570_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51617_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51617_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51640_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51640_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51645_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51645_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51647_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51647_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51651_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51651_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51652_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51652_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51659_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51659_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51668_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51668_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51669_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51669_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51677_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 51677_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 51682_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51682_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51685_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51685_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51686_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51686_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51700_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51700_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51703_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51703_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51707_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51707_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51710_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51710_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51713_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51713_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51717_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51717_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51722_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51722_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51723_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51723_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 51751_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 51751_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
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Considering the candidate 16861_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
Preparing report for the candidate 16861_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
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Considering the candidate 29370_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453
The candidate 29370_fd_Psc-03-Q2b1x1_2026-09-06_05-48-29_20.00sec_0.00C_LIGHT_0453 did not pass the final checks
