This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5
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 07.4401 2461290.9401 11.71 02:15:37.61 +12:42:43.5
152.76196 -45.22778 galactic Ari Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -0 -0 0 11.8 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:37.61 +12:42:43.5: 15.45 +/- 0.25 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:37.61 +12:42:43.5: 15.37 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.41 +/- 0.18
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 07.4401* 02 15 37.61 +12 42 43.5 11.7 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,2461290.9401,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 11.71CV 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 07.4401 2461290.9401 12.42 01:45:36.42 +10:28:14.3
144.00223 -50.17190 galactic Psc Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.124 Alkeste -0 0 0 12.5 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:36.42 +10:28:14.3: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:36.42 +10:28:14.3: 16.01 +/- 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,2461290.9401,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 12.42CV 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 07.4401 2461290.9401 13.73 01:54:50.20 +15:58:08.5
144.43232 -44.23992 galactic Ari Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.295 Theresia 0 0 1 14.0 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:50.20 +15:58:08.5: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:50.20 +15:58:08.5: 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!
TCP 2026 09 07.4401* 01 54 50.20 +15 58 08.5 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,2461290.9401,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 13.73CV 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 07.4401 2461290.9401 13.72 01:54:11.67 +13:50:25.3
145.26507 -46.29222 galactic Ari Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.147 Protogeneia -0 -0 0 13.8 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:11.67 +13:50:25.3: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:11.67 +13:50:25.3: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.4401* 01 54 11.67 +13 50 25.3 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,2461290.9401,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 13.72CV 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 07.4401 2461290.9401 13.76 01:54:59.61 +10:09:37.1
147.52870 -49.65191 galactic Psc Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.167 Urda -0 -0 0 14.0 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:59.61 +10:09:37.1: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:59.61 +10:09:37.1: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461290.9401,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 13.76CV 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 07.4401 2461290.9401 13.93 01:39:19.24 +15:12:13.1
139.70993 -46.10238 galactic Psc Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.517 Edith 0 0 0 14.0 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:19.24 +15:12:13.1: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:19.24 +15:12:13.1: 16.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461290.9401,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 13.93CV 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 07.4401 2461290.9401 14.04 01:53:35.62 +14:47:02.1
144.60246 -45.45636 galactic Ari Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1572 Posnania -1 0 1 14.4 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:35.62 +14:47:02.1: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:35.62 +14:47:02.1: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.4401* 01 53 35.62 +14 47 02.1 14.0 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,2461290.9401,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 14.04CV 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 07.4401 2461290.9401 14.22 02:07:42.94 +10:37:55.2
151.58035 -47.95156 galactic Ari Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.401 Ottilia 0 0 1 14.8 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:07:42.94 +10:37:55.2: 15.96 +/- 0.35 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:07:42.94 +10:37:55.2: 15.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.96 +/- 0.35
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 07.4401* 02 07 42.94 +10 37 55.2 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,2461290.9401,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 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 07.4401 2461290.9401 14.91 01:40:18.68 +19:11:26.1
138.58267 -42.19107 galactic Psc Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.661 Cloelia -1 -1 1 14.8 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:18.68 +19:11:26.1: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:40:18.68 +19:11:26.1: 15.91 +/- 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,2461290.9401,14.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 14.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.4401 2461290.9401 15.07 01:58:29.15 +12:27:37.2
147.41687 -47.19886 galactic Ari Second-epoch detections are separated by 2.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2675 Tolkien 0 1 1 15.2 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:58:29.15 +12:27:37.2: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:58:29.15 +12:27:37.2: 16.03 +/- 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 07.4401* 01 58 29.15 +12 27 37.2 15.1 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,2461290.9401,15.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260907.4401 15.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461290.94045516 07.09.2026 10:34:05.326 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8170
Objects passed selection criteria: 8160
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: 7649.5
Average stars matched: 7340.75 (95.9638 %)
Memory usage VmPeak: 234044 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 Mon Sep 7 05:35:52 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461290.94045516 07.09.2026 10:34:05.326 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 79
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 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): 39633
Objects passed selection criteria: 39534
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: 37962.5
Average stars matched: 36857.5 (97.0892 %)
Memory usage VmPeak: 260328 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 Mon Sep 7 05:36:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.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: 2461290.93972465
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.869 +14:00:12.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:40.469 +14:00:14.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:40.469 +14:00:14.76
Angular distance between the image centers 0.0025 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:38.422 +14:00:47.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:38.422 +14:00:47.26
Angular distance between the image centers 0.0113 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:46:40.469 +14:00:14.76
Second-epoch second image center 01:46:38.422 +14:00:47.26
Angular distance between the image centers 0.01225 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.MfYAsxbCmL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.9HWUCFPvIg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits &> /tmp/tmp.3ftLsgxEyd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits &> /tmp/tmp.Km50cNNknT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950100
a=0.000000 b=1.000000 c=22.950100
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 deg
Loaded 4730 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=6.0)
Read 6762 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4566 to 34.9567 deg, Dec +8.6053 to +19.2739 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.4566 to 34.9567 deg, Dec 8.6053 to 19.2739 deg
Loaded 4732 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3812 out of 4016 total matches.
Matched with Tycho-2 4016 out of 6762 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.0 pix Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.9 pix fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
2.9 pix fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.2 mag. Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.2 mag. fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
15.2 mag. fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.3 (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.MfYAsxbCmL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, bad_region=0, passed=7679
Got 7679 stars (including 7121 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 7679 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 4873 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4873 sigma_overall_arcsec=0.237 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.223 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.200 n_q1=1261 n_q2=1216 n_q3=1199 n_q4=1197 worst_quadrant_to_overall_ratio=1.365
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.9HWUCFPvIg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=519, bad_region=0, passed=6762
Got 6762 stars (including 6236 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 6762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4878 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.239 n_q1=1250 n_q2=1227 n_q3=1200 n_q4=1201 worst_quadrant_to_overall_ratio=1.449
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.3ftLsgxEyd (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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=396, bad_region=0, passed=8156
Got 8156 stars (including 7751 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat
util/solve_plate_with_UCAC5 got 8156 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 8156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 8156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 8156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4872 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4872 robust_rms=10.478 arcsec worst_quadrant_rms=11.679 arcsec
SIP_REFIT: SIP order 3 trial: matched=4872 robust_rms=0.339 arcsec worst_quadrant_rms=0.359 arcsec
SIP_REFIT: SIP order 5 trial: matched=4872 robust_rms=0.249 arcsec worst_quadrant_rms=0.262 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4872 robust_rms_before=1.046 arcsec robust_rms_before_corrected=0.255 arcsec robust_rms_after=0.249 arcsec worst_quadrant_rms_before=0.276 worst_quadrant_rms_after=0.262
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.276 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits N_match=4872 sigma_overall_arcsec=0.266 sigma_q1_arcsec=0.272 sigma_q2_arcsec=0.288 sigma_q3_arcsec=0.241 sigma_q4_arcsec=0.251 n_q1=1319 n_q2=1186 n_q3=1207 n_q4=1160 worst_quadrant_to_overall_ratio=1.082
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits -region wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.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.Km50cNNknT (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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=411, bad_region=0, passed=8198
Got 8198 stars (including 7777 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat
util/solve_plate_with_UCAC5 got 8198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
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: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 8198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
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(), 8198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 8198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4873 robust_rms=10.500 arcsec worst_quadrant_rms=11.941 arcsec
SIP_REFIT: SIP order 3 trial: matched=4873 robust_rms=0.318 arcsec worst_quadrant_rms=0.336 arcsec
SIP_REFIT: SIP order 5 trial: matched=4873 robust_rms=0.244 arcsec worst_quadrant_rms=0.252 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4873 robust_rms_before=1.028 arcsec robust_rms_before_corrected=0.252 arcsec robust_rms_after=0.244 arcsec worst_quadrant_rms_before=0.265 worst_quadrant_rms_after=0.252
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.265 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits N_match=4873 sigma_overall_arcsec=0.257 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.280 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.236 n_q1=1322 n_q2=1180 n_q3=1208 n_q4=1163 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits -region wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
Saving the final (post-refit) wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits sigma_overall=0.237 worst_q_ratio=1.365
ref2=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits sigma_overall=0.294 worst_q_ratio=1.449
new1=fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits sigma_overall=0.266 worst_q_ratio=1.082
new2=fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits sigma_overall=0.257 worst_q_ratio=1.091
reference average sigma_overall=0.2655 worst_q_ratio=1.407
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_astrometric_residuals.png (4873 matched stars from wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.21 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139_astrometric_residuals.png (4878 matched stars from wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442_astrometric_residuals.png (4872 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443_astrometric_residuals.png (4873 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits'
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:40.29 +14:47:44.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:16.02 +15:47:07.6: 12.45 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:37.61 +12:42:43.5: 15.45 +/- 0.25 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:47:14.18 +15:15:20.8: 12.49 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:51:34.80 +14:41:58.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:52:41.77 +15:04:49.5: 12.40 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:30.21 +15:21:57.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:57:53.88 +14:23:11.1: 12.39 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:07.92 +14:51:02.8: 12.45 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:03.02 +16:18:33.4: 12.47 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:52:16.02 +15:47:07.6: 12.46 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:51:34.80 +14:41:58.9: 12.46 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:47:14.18 +15:15:20.8: 12.47 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:37.61 +12:42:43.5: 15.37 +/- 0.27 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:50:30.21 +15:21:57.9: 12.44 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:07.92 +14:51:02.8: 12.43 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:57:53.88 +14:23:11.1: 12.41 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:40.29 +14:47:44.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:52:41.77 +15:04:49.5: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 01:52:16.02 +15:47:07.6: ref_mag=12.45 +/- 0.01 new_mean_mag=12.3920 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 01:51:34.80 +14:41:58.9: ref_mag=12.48 +/- 0.01 new_mean_mag=12.4248 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry reference-image weighted average: 15.41 +/- 0.18
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter REJECTED candidate at 01:53:07.92 +14:51:02.8: ref_mag=12.44 +/- 0.01 new_mean_mag=12.4044 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:50:30.21 +15:21:57.9: ref_mag=12.46 +/- 0.01 new_mean_mag=12.4084 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:47:14.18 +15:15:20.8: ref_mag=12.48 +/- 0.01 new_mean_mag=12.4402 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:53:40.29 +14:47:44.9: ref_mag=12.45 +/- 0.01 new_mean_mag=12.4267 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:57:53.88 +14:23:11.1: ref_mag=12.40 +/- 0.01 new_mean_mag=12.3782 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:52:41.77 +15:04:49.5: ref_mag=12.40 +/- 0.01 new_mean_mag=12.3359 delta=0.06 (need > 0.90)
Forced photometry filter KEPT candidate at 02:15:37.61 +12:42:43.5: ref_mag=15.41 +/- 0.18 new_mean_mag=11.7172 delta=3.69 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:03.02 +16:18:33.4: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter REJECTED candidate at 01:53:03.02 +16:18:33.4: ref_mag=12.47 +/- 0.01 new_mean_mag=12.4406 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:50.98 +13:35:29.0: 12.51 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:57.88 +16:10:54.6: 12.46 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:50.98 +13:35:29.0: 12.53 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:42:57.88 +16:10:54.6: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter REJECTED candidate at 01:53:50.98 +13:35:29.0: ref_mag=12.52 +/- 0.01 new_mean_mag=12.4517 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 01:42:57.88 +16:10:54.6: ref_mag=12.45 +/- 0.01 new_mean_mag=12.4437 delta=0.01 (need > 0.90)
Adding exclusion_list_local.txt__out20184.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20184_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 20184_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20242_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20242_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
**** FOUND 02:10:13.50 +11:31:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20250_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20250_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20251_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20251_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20260_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20260_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20262_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20262_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20263_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20263_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20264_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20264_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20266_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20266_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20267_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20267_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20269_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20269_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20270_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20270_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20271_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 20271_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:15:37.61 +12:42:43.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.869 +14:00:12.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:40.469 +14:00:14.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:40.469 +14:00:14.76
Angular distance between the image centers 0.0025 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:38.422 +14:00:47.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:38.422 +14:00:47.26
Angular distance between the image centers 0.0113 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:46:40.469 +14:00:14.76
Second-epoch second image center 01:46:38.422 +14:00:47.26
Angular distance between the image centers 0.01225 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.Xo2qpi0fTc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.hLGuCrocQh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits &> /tmp/tmp.pgkRWxU3IS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits &> /tmp/tmp.j9fO5yVLyB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.860050
a=0.000000 b=1.000000 c=22.860050
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=4.9)
Read 38153 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4016 to 34.9977 deg, Dec +8.5904 to +19.2796 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 18.4016 to 34.9977 deg, Dec 8.5904 to 19.2796 deg
Loaded 4774 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3712 out of 4109 total matches.
Matched with Tycho-2 4109 out of 38153 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 72 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
1.9 pix Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.7 pix fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
2.7 pix fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Limiting magnitude estimates:
15.5 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.4 mag. Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.3 mag. fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
15.3 mag. fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Xo2qpi0fTc (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1873, bad_region=4, passed=40626
Got 40626 stars (including 38681 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 40626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 40626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4878 sigma_overall_arcsec=0.229 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.218 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.197 n_q1=1241 n_q2=1253 n_q3=1190 n_q4=1194 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hLGuCrocQh (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1585, bad_region=24, passed=38135
Got 38135 stars (including 36454 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 38135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 4881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 38135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4881 stars left (next iteration limit 5369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4881 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.264 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.238 n_q1=1246 n_q2=1250 n_q3=1199 n_q4=1186 worst_quadrant_to_overall_ratio=1.439
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.pgkRWxU3IS (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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1395, bad_region=44, passed=37052
Got 37052 stars (including 35569 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat
util/solve_plate_with_UCAC5 got 37052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 37052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 4878 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(), 37052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 37052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.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=10.746 arcsec worst_quadrant_rms=12.139 arcsec
SIP_REFIT: SIP order 3 trial: matched=4876 robust_rms=0.338 arcsec worst_quadrant_rms=0.355 arcsec
SIP_REFIT: SIP order 5 trial: matched=4876 robust_rms=0.247 arcsec worst_quadrant_rms=0.258 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4876 robust_rms_before=1.056 arcsec robust_rms_before_corrected=0.256 arcsec robust_rms_after=0.247 arcsec worst_quadrant_rms_before=0.270 worst_quadrant_rms_after=0.258
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.270 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits N_match=4876 sigma_overall_arcsec=0.264 sigma_q1_arcsec=0.278 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.233 sigma_q4_arcsec=0.247 n_q1=1318 n_q2=1192 n_q3=1203 n_q4=1163 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits -region wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.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.j9fO5yVLyB (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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1450, bad_region=44, passed=37016
Got 37016 stars (including 35479 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat
util/solve_plate_with_UCAC5 got 37016 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.6)
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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 37016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.6)
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(), 37016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 37016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.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=10.732 arcsec worst_quadrant_rms=12.183 arcsec
SIP_REFIT: SIP order 3 trial: matched=4876 robust_rms=0.317 arcsec worst_quadrant_rms=0.329 arcsec
SIP_REFIT: SIP order 5 trial: matched=4876 robust_rms=0.244 arcsec worst_quadrant_rms=0.251 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4876 robust_rms_before=1.039 arcsec robust_rms_before_corrected=0.254 arcsec robust_rms_after=0.244 arcsec worst_quadrant_rms_before=0.270 worst_quadrant_rms_after=0.251
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.270 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits N_match=4876 sigma_overall_arcsec=0.261 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.279 sigma_q3_arcsec=0.237 sigma_q4_arcsec=0.241 n_q1=1316 n_q2=1197 n_q3=1204 n_q4=1159 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits -region wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-33-02_20.00sec_-0.00C_LIGHTs_0442.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.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_2026-09-07_CI_Psc-03-Q1b1x1_053446_TTUQ1b1x1_806917_IcLcgfW5/wcs_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443.fits
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:21:26.13 +14:47:14.4: 14.86 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:36.42 +10:28:14.3: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:13:49.97 +13:47:05.3: 14.67 +/- 0.10 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:37:59.21 +18:28:10.3: 14.31 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:17:00.81 +12:20:14.0: 14.37 +/- 0.09 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:00.88 +17:49:34.8: 14.51 +/- 0.09 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:17.10 +17:31:16.8: 13.65 +/- 0.04 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:55.74 +18:59:51.2: 14.00 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:50.20 +15:58:08.5: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:02:54.83 +16:41:57.7: 13.44 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:55.74 +18:59:51.2: 14.06 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:17:00.81 +12:20:14.0: 14.46 +/- 0.12 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:00.88 +17:49:34.8: 14.41 +/- 0.10 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:36.42 +10:28:14.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:13:49.97 +13:47:05.3: 14.82 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:37:59.21 +18:28:10.3: 14.57 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:17.10 +17:31:16.8: 13.71 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:21:26.13 +14:47:14.4: 14.87 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Forced photometry reference-image weighted average: 14.40 +/- 0.07
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry reference-image weighted average: 14.40 +/- 0.07
Forced photometry reference-image weighted average: 14.46 +/- 0.07
Forced photometry reference-image weighted average: 14.73 +/- 0.08
Forced photometry reference-image weighted average: 14.87 +/- 0.10
Forced photometry filter REJECTED candidate at 01:31:55.74 +18:59:51.2: ref_mag=14.02 +/- 0.04 new_mean_mag=14.1544 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:17:00.81 +12:20:14.0: ref_mag=14.40 +/- 0.07 new_mean_mag=14.4347 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:31:17.10 +17:31:16.8: ref_mag=13.67 +/- 0.03 new_mean_mag=14.0285 delta=-0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:37:59.21 +18:28:10.3: ref_mag=14.40 +/- 0.07 new_mean_mag=14.4416 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:21:26.13 +14:47:14.4: ref_mag=14.87 +/- 0.10 new_mean_mag=14.7924 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:13:49.97 +13:47:05.3: ref_mag=14.73 +/- 0.08 new_mean_mag=14.6145 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:28:00.88 +17:49:34.8: ref_mag=14.46 +/- 0.07 new_mean_mag=14.5476 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:50.20 +15:58:08.5: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:02:54.83 +16:41:57.7: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter REJECTED candidate at 02:02:54.83 +16:41:57.7: ref_mag=13.46 +/- 0.03 new_mean_mag=13.6910 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:07:42.94 +10:37:55.2: 15.96 +/- 0.35 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:59.61 +10:09:37.1: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:11.67 +13:50:25.3: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:35.62 +14:47:02.1: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:19.24 +15:12:13.1: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:01:36.18 +14:32:26.7: 14.09 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:15:38.24 +09:18:22.8: 14.79 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:59.61 +10:09:37.1: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:07:42.94 +10:37:55.2: 15.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.96 +/- 0.35
Forced photometry filter KEPT candidate at 02:07:42.94 +10:37:55.2: ref_mag=15.96 +/- 0.35 new_mean_mag=14.2190 delta=1.74 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:11.67 +13:50:25.3: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:35.62 +14:47:02.1: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:19.24 +15:12:13.1: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:58.45 +14:22:00.6: 14.33 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:01:36.18 +14:32:26.7: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Forced photometry filter REJECTED candidate at 02:01:36.18 +14:32:26.7: ref_mag=14.12 +/- 0.05 new_mean_mag=14.2490 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:15:38.24 +09:18:22.8: 14.46 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.10
Forced photometry filter REJECTED candidate at 01:15:38.24 +09:18:22.8: ref_mag=14.60 +/- 0.10 new_mean_mag=14.3288 delta=0.27 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:58.45 +14:22:00.6: 14.38 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.06
Forced photometry filter REJECTED candidate at 01:34:58.45 +14:22:00.6: ref_mag=14.35 +/- 0.06 new_mean_mag=14.4844 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:26:01.95 +09:18:28.4: 14.57 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:15:16.61 +14:36:24.1: 14.67 +/- 0.12 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:24:12.35 +16:38:02.8: 14.62 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:26:01.95 +09:18:28.4: 14.62 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.08
Forced photometry filter REJECTED candidate at 01:26:01.95 +09:18:28.4: ref_mag=14.59 +/- 0.08 new_mean_mag=14.3690 delta=0.22 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:15:16.61 +14:36:24.1: 14.53 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.09
Forced photometry filter REJECTED candidate at 01:15:16.61 +14:36:24.1: ref_mag=14.60 +/- 0.09 new_mean_mag=14.5115 delta=0.09 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:24:12.35 +16:38:02.8: 14.42 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.08
Forced photometry filter REJECTED candidate at 01:24:12.35 +16:38:02.8: ref_mag=14.52 +/- 0.08 new_mean_mag=14.5136 delta=0.00 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:24:14.82 +12:53:40.6: 14.62 +/- 0.12 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:23:40.68 +09:44:36.2: 15.26 +/- 0.21 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:18:35.69 +17:41:26.6: 14.84 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:24:14.82 +12:53:40.6: 14.87 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:23:40.68 +09:44:36.2: 14.78 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.09
Forced photometry filter REJECTED candidate at 01:24:14.82 +12:53:40.6: ref_mag=14.71 +/- 0.09 new_mean_mag=14.5590 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 14.95 +/- 0.12
Forced photometry filter REJECTED candidate at 01:23:40.68 +09:44:36.2: ref_mag=14.95 +/- 0.12 new_mean_mag=14.6345 delta=0.31 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:18:35.69 +17:41:26.6: 14.53 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.09
Forced photometry filter REJECTED candidate at 01:18:35.69 +17:41:26.6: ref_mag=14.66 +/- 0.09 new_mean_mag=14.4096 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:56:57.84 +17:48:59.8: 14.43 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:52.14 +13:46:26.5: 14.62 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:31.02 +13:32:26.8: 14.89 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:56:57.84 +17:48:59.8: 14.45 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.06
Forced photometry filter REJECTED candidate at 01:56:57.84 +17:48:59.8: ref_mag=14.44 +/- 0.06 new_mean_mag=14.6100 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:52.14 +13:46:26.5: 14.83 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.07
Forced photometry filter REJECTED candidate at 01:45:52.14 +13:46:26.5: ref_mag=14.69 +/- 0.07 new_mean_mag=14.6483 delta=0.04 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:19:31.02 +13:32:26.8: 14.97 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.11
Forced photometry filter REJECTED candidate at 01:19:31.02 +13:32:26.8: ref_mag=14.92 +/- 0.11 new_mean_mag=14.7141 delta=0.21 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:36:20.44 +14:59:59.4: 14.77 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:23:14.64 +13:42:27.9: 15.04 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:25:21.39 +16:20:27.1: 15.34 +/- 0.20 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:36:20.44 +14:59:59.4: 14.91 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.08
Forced photometry filter REJECTED candidate at 01:36:20.44 +14:59:59.4: ref_mag=14.82 +/- 0.08 new_mean_mag=14.7729 delta=0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:23:14.64 +13:42:27.9: 15.28 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.13
Forced photometry filter REJECTED candidate at 01:23:14.64 +13:42:27.9: ref_mag=15.12 +/- 0.13 new_mean_mag=14.8612 delta=0.26 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:25:21.39 +16:20:27.1: 14.99 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.13
Forced photometry filter REJECTED candidate at 01:25:21.39 +16:20:27.1: ref_mag=15.13 +/- 0.13 new_mean_mag=14.8371 delta=0.30 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:34.48 +09:19:14.9: 14.93 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:42.67 +11:27:21.5: 15.11 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:57.06 +10:15:18.0: 15.19 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:19:34.48 +09:19:14.9: 15.13 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.13
Forced photometry filter REJECTED candidate at 01:19:34.48 +09:19:14.9: ref_mag=15.00 +/- 0.13 new_mean_mag=14.8139 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:16:42.67 +11:27:21.5: 14.80 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.12
Forced photometry filter REJECTED candidate at 01:16:42.67 +11:27:21.5: ref_mag=14.93 +/- 0.12 new_mean_mag=14.8475 delta=0.08 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:57.06 +10:15:18.0: 15.26 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.22 +/- 0.14
Forced photometry filter REJECTED candidate at 02:15:57.06 +10:15:18.0: ref_mag=15.22 +/- 0.14 new_mean_mag=14.9485 delta=0.27 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:54.33 +14:32:31.5: 14.93 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:20:02.13 +14:57:11.0: 15.14 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:18.68 +19:11:26.1: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:20:02.13 +14:57:11.0: 15.00 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:16:54.33 +14:32:31.5: 15.03 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.13
Forced photometry filter REJECTED candidate at 01:20:02.13 +14:57:11.0: ref_mag=15.07 +/- 0.13 new_mean_mag=14.8672 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 14.97 +/- 0.12
Forced photometry filter REJECTED candidate at 01:16:54.33 +14:32:31.5: ref_mag=14.97 +/- 0.12 new_mean_mag=14.7123 delta=0.26 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:40:18.68 +19:11:26.1: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:19.18 +10:17:27.4: 15.12 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:23.67 +12:56:47.0: 15.44 +/- 0.24 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:19.18 +10:17:27.4: 15.54 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.12
Forced photometry filter REJECTED candidate at 01:53:19.18 +10:17:27.4: ref_mag=15.24 +/- 0.12 new_mean_mag=14.9907 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:16:23.67 +12:56:47.0: 15.24 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.17
Forced photometry filter REJECTED candidate at 01:16:23.67 +12:56:47.0: ref_mag=15.33 +/- 0.17 new_mean_mag=14.8599 delta=0.47 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:42.07 +12:36:41.6: 14.99 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:23:01.42 +13:43:44.1: 14.86 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:16:42.07 +12:36:41.6: 14.84 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.11
Forced photometry filter REJECTED candidate at 01:16:42.07 +12:36:41.6: ref_mag=14.92 +/- 0.11 new_mean_mag=14.9613 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:23:01.42 +13:43:44.1: 14.69 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.09
Forced photometry filter REJECTED candidate at 01:23:01.42 +13:43:44.1: ref_mag=14.76 +/- 0.09 new_mean_mag=14.7782 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:21:30.62 +16:12:50.9: 15.02 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:27:37.87 +10:58:49.0: 15.02 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:21:30.62 +16:12:50.9: 14.90 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.11
Forced photometry filter REJECTED candidate at 01:21:30.62 +16:12:50.9: ref_mag=14.96 +/- 0.11 new_mean_mag=14.7791 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:27:37.87 +10:58:49.0: 15.41 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.12
Forced photometry filter REJECTED candidate at 01:27:37.87 +10:58:49.0: ref_mag=15.13 +/- 0.12 new_mean_mag=14.8788 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:23.55 +16:14:45.0: 15.05 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:22.16 +18:44:32.0: 14.92 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:24:01.59 +18:00:57.0: 15.02 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:35:54.04 +10:13:38.4: 15.12 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:23:44.34 +10:59:53.7: 15.16 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:21:17.86 +13:57:26.7: 15.14 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:58:29.15 +12:27:37.2: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:23.55 +16:14:45.0: 15.13 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.11
Forced photometry filter REJECTED candidate at 01:28:23.55 +16:14:45.0: ref_mag=15.08 +/- 0.11 new_mean_mag=14.8453 delta=0.24 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:41:22.16 +18:44:32.0: 15.03 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.10
Forced photometry filter REJECTED candidate at 01:41:22.16 +18:44:32.0: ref_mag=14.96 +/- 0.10 new_mean_mag=14.7438 delta=0.22 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:25:36.57 +18:26:42.1: 14.85 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:18:15.86 +12:24:36.3: 15.33 +/- 0.21 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:24:01.59 +18:00:57.0: 15.17 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.12
Forced photometry filter REJECTED candidate at 01:24:01.59 +18:00:57.0: ref_mag=15.08 +/- 0.12 new_mean_mag=14.8931 delta=0.18 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:35:54.04 +10:13:38.4: 15.03 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.11
Forced photometry filter REJECTED candidate at 01:35:54.04 +10:13:38.4: ref_mag=15.08 +/- 0.11 new_mean_mag=14.9350 delta=0.14 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:23:44.34 +10:59:53.7: 15.12 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.13
Forced photometry filter REJECTED candidate at 01:23:44.34 +10:59:53.7: ref_mag=15.14 +/- 0.13 new_mean_mag=14.8801 delta=0.26 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:21:17.86 +13:57:26.7: 15.34 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.14
Forced photometry filter REJECTED candidate at 01:21:17.86 +13:57:26.7: ref_mag=15.21 +/- 0.14 new_mean_mag=14.9561 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:58:29.15 +12:27:37.2: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:18:15.86 +12:24:36.3: 15.22 +/- 0.23 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:25:36.57 +18:26:42.1: 15.02 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.16
Forced photometry reference-image weighted average: 14.91 +/- 0.11
Forced photometry filter REJECTED candidate at 01:18:15.86 +12:24:36.3: ref_mag=15.28 +/- 0.16 new_mean_mag=14.9698 delta=0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:25:36.57 +18:26:42.1: ref_mag=14.91 +/- 0.11 new_mean_mag=14.9522 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:02.35 +15:18:00.3: 15.22 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:27:59.30 +10:56:21.1: 14.99 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:09.30 +09:32:34.0: 15.71 +/- 0.26 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:32.81 +14:41:34.6: 15.37 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:03.11 +15:19:30.5: 15.08 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:40:26.73 +09:35:47.7: 15.18 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:16:02.35 +15:18:00.3: 15.24 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.15
Forced photometry filter REJECTED candidate at 01:16:02.35 +15:18:00.3: ref_mag=15.23 +/- 0.15 new_mean_mag=14.8467 delta=0.38 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:27:59.30 +10:56:21.1: 14.73 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.09
Forced photometry filter REJECTED candidate at 01:27:59.30 +10:56:21.1: ref_mag=14.84 +/- 0.09 new_mean_mag=14.9180 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:46:14.98 +11:58:32.7: 15.23 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:40:09.30 +09:32:34.0: 15.28 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.43 +/- 0.15
Forced photometry filter REJECTED candidate at 01:40:09.30 +09:32:34.0: ref_mag=15.43 +/- 0.15 new_mean_mag=15.0027 delta=0.43 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:41.85 +09:38:58.8: 15.22 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:32.81 +14:41:34.6: 15.14 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.13
Forced photometry filter REJECTED candidate at 01:34:32.81 +14:41:34.6: ref_mag=15.24 +/- 0.13 new_mean_mag=14.9531 delta=0.29 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:19:03.11 +15:19:30.5: 15.06 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.12
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:40:26.73 +09:35:47.7: 15.18 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 01:19:03.11 +15:19:30.5: ref_mag=15.07 +/- 0.12 new_mean_mag=14.9715 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 15.18 +/- 0.12
Forced photometry filter REJECTED candidate at 01:40:26.73 +09:35:47.7: ref_mag=15.18 +/- 0.12 new_mean_mag=14.9521 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:46:14.98 +11:58:32.7: 15.38 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.12
Forced photometry filter REJECTED candidate at 01:46:14.98 +11:58:32.7: ref_mag=15.29 +/- 0.12 new_mean_mag=15.0913 delta=0.20 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:41:41.85 +09:38:58.8: 15.48 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.14
Forced photometry filter REJECTED candidate at 01:41:41.85 +09:38:58.8: ref_mag=15.31 +/- 0.14 new_mean_mag=15.0428 delta=0.27 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:26:53.64 +18:49:46.3: 15.02 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:33:26.30 +15:08:24.0: 15.43 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:32:09.58 +18:22:32.4: 15.12 +/- 0.15 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:02.72 +17:25:06.6: 15.22 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:23:36.91 +12:18:11.3: 15.40 +/- 0.21 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:22:36.64 +12:16:36.5: 15.26 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:26:53.64 +18:49:46.3: 15.34 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.13
Forced photometry filter REJECTED candidate at 01:26:53.64 +18:49:46.3: ref_mag=15.11 +/- 0.13 new_mean_mag=14.9444 delta=0.17 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:33:26.30 +15:08:24.0: 15.61 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.49 +/- 0.15
Forced photometry filter REJECTED candidate at 01:33:26.30 +15:08:24.0: ref_mag=15.49 +/- 0.15 new_mean_mag=15.1216 delta=0.37 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:32:09.58 +18:22:32.4: 15.21 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.12
Forced photometry filter REJECTED candidate at 01:32:09.58 +18:22:32.4: ref_mag=15.15 +/- 0.12 new_mean_mag=14.8463 delta=0.31 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:02.72 +17:25:06.6: 15.31 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.13
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:23:36.91 +12:18:11.3: 15.00 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 01:28:02.72 +17:25:06.6: ref_mag=15.26 +/- 0.13 new_mean_mag=15.0291 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:22:36.64 +12:16:36.5: 15.63 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.13
Forced photometry filter REJECTED candidate at 01:23:36.91 +12:18:11.3: ref_mag=15.16 +/- 0.13 new_mean_mag=14.9770 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 15.37 +/- 0.16
Forced photometry filter REJECTED candidate at 01:22:36.64 +12:16:36.5: ref_mag=15.37 +/- 0.16 new_mean_mag=15.0665 delta=0.30 (need > 0.90)
Adding exclusion_list_local.txt__out51849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52827.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 51656_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 51656_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 51662_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 51662_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 51664_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 51664_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 51667_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 51667_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 51669_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 51669_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 51673_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 51673_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 51674_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 51674_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 51849_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 51849_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52113_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52113_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
**** FOUND 01:47:13.24 +17:54:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52127_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52127_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
**** FOUND 01:39:44.53 +16:26:02.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52130_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52130_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52138_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52138_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52142_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52142_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52151_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52151_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52257_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52257_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
**** FOUND 01:43:42.62 +12:53:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52258_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52258_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52272_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52272_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
**** FOUND 02:02:42.90 +13:27:58.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52307_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52307_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52331_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52331_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52345_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52345_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52377_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52377_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
**** FOUND 01:25:56.27 +16:36:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52449_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52449_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52464_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52464_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52482_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52482_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52517_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52517_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52529_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52529_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52545_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52545_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52565_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52565_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52571_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52571_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52647_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52647_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52648_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52648_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52662_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52662_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52689_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52689_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52700_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52700_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52706_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52706_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52707_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52707_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52719_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52719_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52724_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52724_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52731_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52731_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52733_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52733_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52735_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52735_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52739_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52739_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52757_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52757_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52761_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52761_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52771_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52771_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52781_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52781_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52784_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52784_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52785_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52785_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52787_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52787_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52801_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52801_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52806_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52806_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52812_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52812_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52822_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52822_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52827_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
Preparing report for the candidate 52827_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
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Considering the candidate 52829_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52829_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52832_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52832_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52838_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52838_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52840_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52840_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52842_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52842_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52848_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52848_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52850_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52850_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52853_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52853_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52878_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52878_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52880_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52880_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52891_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52891_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52898_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52898_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52902_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52902_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52924_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52924_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52934_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52934_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 52941_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 52941_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
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Considering the candidate 29370_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 29370_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
**** FOUND 02:00:56.16 +09:45:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33697_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443
The candidate 33697_fd_Psc-03-Q1b1x1_2026-09-07_05-34-05_20.00sec_-0.00C_LIGHTs_0443 did not pass the final checks
