This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr
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 07 23.4165 2461244.9165 12.47 01:32:46.05 +13:16:17.5
138.16806 -48.37377 galactic Psc Second-epoch detections are separated by 0.5" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.101 Helena -2 -1 2 12.8 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:32:46.05 +13:16:17.5: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:32:46.05 +13:16:17.5: 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,2461244.9165,12.47,0.05,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 20260723.4165 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4165 2461244.9165 12.70 01:39:04.75 +10:27:50.9
141.60865 -50.67191 galactic Psc Second-epoch detections are separated by 0.6" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -1 -0 1 12.6 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:04.75 +10:27:50.9: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:39:04.75 +10:27:50.9: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461244.9165,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260723.4165 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4165 2461244.9165 13.07 01:34:29.07 +10:07:18.8
140.03481 -51.31476 galactic Psc Second-epoch detections are separated by 0.7" and 9.1 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 1 13.2 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:29.07 +10:07:18.8: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:34:29.07 +10:07:18.8: 15.77 +/- 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,2461244.9165,13.07,0.05,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 20260723.4165 13.07CV 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
Mean magnitude and position on the discovery images:
2026 07 23.4165 2461244.9165 13.72 01:30:43.09 +13:30:11.0
137.35784 -48.26539 galactic Psc Second-epoch detections are separated by 0.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.212 Medea -1 -0 1 13.9 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:43.09 +13:30:11.0: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:30:43.09 +13:30:11.0: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461244.9165,13.72,0.05,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 20260723.4165 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 07 23.4165 2461244.9165 14.40 01:50:38.79 +16:45:00.1
142.75563 -43.83086 galactic Ari Second-epoch detections are separated by 0.1" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.297 Caecilia -1 -0 1 14.6 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:38.79 +16:45:00.1: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:50:38.79 +16:45:00.1: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 23.4165* 01 50 38.79 +16 45 00.1 14.4 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,2461244.9165,14.40,0.05,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 20260723.4165 14.40CV 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 07 23.4165 2461244.9165 14.44 01:31:46.87 +18:57:38.0
135.99582 -42.88550 galactic Psc Second-epoch detections are separated by 2.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.760 Massinga -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 01:31:46.87 +18:57:38.0: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:31:46.87 +18:57:38.0: 15.80 +/- 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,2461244.9165,14.44,0.05,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 20260723.4165 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4165 2461244.9165 14.60 01:42:46.89 +12:33:00.8
142.00007 -48.41142 galactic Psc Second-epoch detections are separated by 3.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.147 Protogeneia -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 01:42:46.89 +12:33:00.8: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:42:46.89 +12:33:00.8: 16.02 +/- 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,2461244.9165,14.60,0.05,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 20260723.4165 14.60CV 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 07 23.4165 2461244.9165 14.70 01:24:42.12 +12:47:25.2
135.41644 -49.27339 galactic Psc Second-epoch detections are separated by 4.5" and 9.7 pix
The object was found in VSX23" Gaia DR3 2586723326228039040
Type: ROT
# Max. Min./Amp. JD0 Period
16.140 G 16.180 G K
The object was found in astcheck.517 Edith 1 -1 1 14.9 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:24:42.12 +12:47:25.2: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:24:42.12 +12:47:25.2: 15.77 +/- 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
Gaia DR3 2586723326228039040,2461244.9165,14.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2586723326228039040 20260723.4165 14.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4165 2461244.9165 14.66 01:41:38.00 +09:39:02.9
142.94787 -51.25969 galactic Psc Second-epoch detections are separated by 3.1" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.167 Urda -1 -1 2 14.7 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:38.00 +09:39:02.9: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:41:38.00 +09:39:02.9: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461244.9165,14.66,0.05,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 20260723.4165 14.66CV 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: 2461244.91676537 23.07.2026 09:59:58.528 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 23 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 7008
Objects passed selection criteria: 7005
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: 6748
Average stars matched: 6674 (98.9034 %)
Memory usage VmPeak: 116080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 22 16:05:55 CDT 2026
VaST build number 1.0rc89-166-g55a66cb7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-22)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 23 05:17:38 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: 2461244.91676537 23.07.2026 09:59:58.528 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 45
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: 28 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 36664
Objects passed selection criteria: 36598
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 34646
Average stars matched: 34108 (98.4472 %)
Memory usage VmPeak: 141936 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 22 16:05:55 CDT 2026
VaST build number 1.0rc89-166-g55a66cb7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-22)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 23 05:21:00 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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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: 2461244.91615345
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
Saving 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'
wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits exists and is non-empty
Saving wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits'
wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits'
wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits'
###################################
# 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: 941.4'x626.9' 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: 01:46:39.828 +14:00:12.80 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_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Image size: 941.2'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: 01:46:45.104 +13:59:06.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:45.104 +13:59:06.49
Angular distance between the image centers 0.0282 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
Image size: 941.2'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: 01:46:48.005 +13:59:39.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:48.005 +13:59:39.76
Angular distance between the image centers 0.0343 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 01:46:45.104 +13:59:06.49
Second-epoch second image center 01:46:48.005 +13:59:39.76
Angular distance between the image centers 0.01493 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.aNu6s9hGfG
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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits &> /tmp/tmp.occoOtkXbY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits &> /tmp/tmp.KSRUMyPOox
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits &> /tmp/tmp.dOSmcMuENz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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 18.3971 to 34.9280 deg, Dec +8.6500 to +19.2744 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 18.3971 to 34.9280 deg, Dec 8.6500 to 19.2744 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): 3854 out of 4067 total matches.
Matched with Tycho-2 4067 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 22.950000
a=0.000000 b=1.000000 c=22.950000
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 18.3971 to 34.9280 deg, Dec +8.6500 to +19.2744 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 18.3971 to 34.9280 deg, Dec 8.6500 to 19.2744 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): 3854 out of 4067 total matches.
Matched with Tycho-2 4067 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: 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 6663 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4568 to 34.9561 deg, Dec +8.6500 to +19.2743 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 18.4568 to 34.9561 deg, Dec 8.6500 to 19.2743 deg
Loaded 4716 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): 3860 out of 4017 total matches.
Matched with Tycho-2 4017 out of 6663 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
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
2.2 pix Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
2.6 pix fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
2.6 pix fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
2.0 pix wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.2 pix wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.1 mag. Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
15.0 mag. fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
15.0 mag. fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.aNu6s9hGfG (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/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'
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: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7491 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=969 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.276 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.216 n_q1=215 n_q2=260 n_q3=251 n_q4=243 worst_quadrant_to_overall_ratio=1.236
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
############ /tmp/tmp.occoOtkXbY (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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=444, bad_region=0, passed=6663
Got 6663 stars (including 6203 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 6663 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits N_match=971 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.230 n_q1=224 n_q2=262 n_q3=251 n_q4=234 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -region wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.KSRUMyPOox (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.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_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.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=353, bad_region=0, passed=6417
Got 6417 stars (including 6060 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat
util/solve_plate_with_UCAC5 got 6417 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6286 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits N_match=972 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.300 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.282 n_q1=230 n_q2=251 n_q3=253 n_q4=238 worst_quadrant_to_overall_ratio=1.032
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dOSmcMuENz (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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=343, bad_region=0, passed=6391
Got 6391 stars (including 6043 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat
util/solve_plate_with_UCAC5 got 6391 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 6259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits N_match=972 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.287 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.278 n_q1=233 n_q2=250 n_q3=256 n_q4=233 worst_quadrant_to_overall_ratio=1.081
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# 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=0.283 worst_q_ratio=1.236
ref2=Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits sigma_overall=0.292 worst_q_ratio=1.186
new1=fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits sigma_overall=0.291 worst_q_ratio=1.032
new2=fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits sigma_overall=0.302 worst_q_ratio=1.081
reference average sigma_overall=0.2875 worst_q_ratio=1.211
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 (969 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 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_astrometric_residuals.png (971 matched stars from wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372_astrometric_residuals.png (972 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373_astrometric_residuals.png (972 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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 01:50:30.20 +15:21:57.7: 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 01:33:27.47 +17:34:08.8: 12.30 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:04:15.24 +11:14:09.2: 11.85 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:50:30.20 +15:21:57.7: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter REJECTED candidate at 01:50:30.20 +15:21:57.7: ref_mag=12.46 +/- 0.01 new_mean_mag=12.4116 delta=0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:33:27.47 +17:34:08.8: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:27.47 +17:34:08.8: ref_mag=12.26 +/- 0.01 new_mean_mag=12.3707 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 02:04:15.24 +11:14:09.2: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter REJECTED candidate at 02:04:15.24 +11:14:09.2: ref_mag=11.81 +/- 0.01 new_mean_mag=12.0590 delta=-0.25 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20062_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 20062_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20063_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 20063_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20064_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 20064_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:28:36.31 +14:39:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20216_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 20216_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 02:10:13.51 +11:32:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20220_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 20220_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04646_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 04646_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:22:58.49 +12:52:03.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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 ####
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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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: 941.4'x626.9' 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: 01:46:39.828 +14:00:12.80 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_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Image size: 941.2'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: 01:46:45.104 +13:59:06.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:45.104 +13:59:06.49
Angular distance between the image centers 0.0282 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
Image size: 941.2'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: 01:46:48.005 +13:59:39.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:48.005 +13:59:39.76
Angular distance between the image centers 0.0343 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 01:46:45.104 +13:59:06.49
Second-epoch second image center 01:46:48.005 +13:59:39.76
Angular distance between the image centers 0.01493 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.LDJD6rjhd1
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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits &> /tmp/tmp.Rj0OKsFNz2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits &> /tmp/tmp.zIemqBd50Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits &> /tmp/tmp.hOhu0fvwcf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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 18.3971 to 34.9782 deg, Dec +8.6329 to +19.2915 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 18.3971 to 34.9782 deg, Dec 8.6329 to 19.2915 deg
Loaded 4751 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): 3680 out of 4108 total matches.
Matched with Tycho-2 4108 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 22.860200
a=0.000000 b=1.000000 c=22.860200
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 18.3971 to 34.9782 deg, Dec +8.6329 to +19.2915 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 18.3971 to 34.9782 deg, Dec 8.6329 to 19.2915 deg
Loaded 4751 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): 3680 out of 4108 total matches.
Matched with Tycho-2 4108 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: 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 35714 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4024 to 35.0127 deg, Dec +8.5911 to +19.2852 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 18.4024 to 35.0127 deg, Dec 8.5911 to 19.2852 deg
Loaded 4781 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): 3749 out of 4114 total matches.
Matched with Tycho-2 4114 out of 35714 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 43 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
2.1 pix Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
2.5 pix fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
2.5 pix fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
2.0 pix wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.1 pix wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Limiting magnitude estimates:
15.5 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.3 mag. Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
15.0 mag. fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
15.0 mag. fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.LDJD6rjhd1 (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/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'
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: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 39711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 39708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 39707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=968 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.278 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.224 n_q1=210 n_q2=268 n_q3=245 n_q4=245 worst_quadrant_to_overall_ratio=1.264
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
############ /tmp/tmp.Rj0OKsFNz2 (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.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=1567, bad_region=1, passed=35697
Got 35697 stars (including 34066 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 35697 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 35006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 35008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 35008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits N_match=969 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.289 sigma_q3_arcsec=0.283 sigma_q4_arcsec=0.249 n_q1=220 n_q2=265 n_q3=246 n_q4=238 worst_quadrant_to_overall_ratio=1.338
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits -region wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zIemqBd50Y (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.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_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.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=2, blended=1052, bad_region=13, passed=31526
Got 31526 stars (including 30417 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat
util/solve_plate_with_UCAC5 got 31526 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 30807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 30807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 30807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits N_match=970 sigma_overall_arcsec=0.284 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.297 n_q1=227 n_q2=247 n_q3=255 n_q4=241 worst_quadrant_to_overall_ratio=1.084
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hOhu0fvwcf (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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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=1067, bad_region=14, passed=31607
Got 31607 stars (including 30489 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat
util/solve_plate_with_UCAC5 got 31607 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 31001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 31003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 31003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits N_match=969 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.275 sigma_q2_arcsec=0.342 sigma_q3_arcsec=0.256 sigma_q4_arcsec=0.283 n_q1=231 n_q2=245 n_q3=259 n_q4=234 worst_quadrant_to_overall_ratio=1.129
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-05_20.00sec_0.00C_LIGHTs_0372.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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_2026-07-23_CI_Psc-03-Q1b1x1_050808_TTUQ1b1x1_3093467_hVkemYtr/wcs_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373.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 01:39:04.75 +10:27:50.9: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:43:06.00 +12:34:13.6: 12.61 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:15:20.09 +13:15:27.5: 14.20 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:25.40 +14:16:56.7: 14.98 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:48.17 +10:41:58.1: 14.42 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:21:10.34 +13:12:02.4: 14.16 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:32:46.05 +13:16:17.5: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:29.07 +10:07:18.8: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:15:20.09 +13:15:27.5: 14.22 +/- 0.10 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:19:25.40 +14:16:56.7: 14.64 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.06
Forced photometry filter REJECTED candidate at 01:15:20.09 +13:15:27.5: ref_mag=14.21 +/- 0.06 new_mean_mag=14.1997 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.80 +/- 0.11
Forced photometry filter REJECTED candidate at 01:19:25.40 +14:16:56.7: ref_mag=14.80 +/- 0.11 new_mean_mag=14.6849 delta=0.11 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:39:04.75 +10:27:50.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:38:48.17 +10:41:58.1: 14.43 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.06
Forced photometry filter REJECTED candidate at 01:38:48.17 +10:41:58.1: ref_mag=14.42 +/- 0.06 new_mean_mag=14.3677 delta=0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:21:10.34 +13:12:02.4: 14.24 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Forced photometry filter REJECTED candidate at 01:21:10.34 +13:12:02.4: ref_mag=14.19 +/- 0.06 new_mean_mag=14.1691 delta=0.02 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:43:06.00 +12:34:13.6: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter REJECTED candidate at 01:43:06.00 +12:34:13.6: ref_mag=12.60 +/- 0.01 new_mean_mag=12.6554 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:32:46.05 +13:16:17.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:34:29.07 +10:07:18.8: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:29:48.54 +14:23:13.4: 13.30 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:33:38.73 +16:08:30.9: 13.84 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:29:48.54 +14:23:13.4: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter REJECTED candidate at 01:29:48.54 +14:23:13.4: ref_mag=13.28 +/- 0.02 new_mean_mag=13.4687 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:43.09 +13:30:11.0: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:33:38.73 +16:08:30.9: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter REJECTED candidate at 01:33:38.73 +16:08:30.9: ref_mag=13.71 +/- 0.03 new_mean_mag=13.7484 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:30:43.09 +13:30:11.0: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:38.79 +16:45:00.1: 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 02:01:36.13 +14:32:26.8: 14.08 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:46.87 +18:57:38.0: 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 01:42:46.89 +12:33:00.8: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:50:38.79 +16:45:00.1: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 02:01:36.13 +14:32:26.8: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.05
Forced photometry filter REJECTED candidate at 02:01:36.13 +14:32:26.8: ref_mag=14.06 +/- 0.05 new_mean_mag=14.2941 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:31:46.87 +18:57:38.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:17:30.10 +12:15:04.2: 14.97 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:42:46.89 +12:33:00.8: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:21:11.84 +16:13:31.6: 14.86 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:17:30.10 +12:15:04.2: 14.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.12
Forced photometry filter REJECTED candidate at 01:17:30.10 +12:15:04.2: ref_mag=14.89 +/- 0.12 new_mean_mag=14.6594 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:21:11.84 +16:13:31.6: 14.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.10
Forced photometry filter REJECTED candidate at 01:21:11.84 +16:13:31.6: ref_mag=14.83 +/- 0.10 new_mean_mag=14.7102 delta=0.12 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:16:31.25 +13:38:34.8: 14.97 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:21:09.29 +13:34:30.2: 15.41 +/- 0.21 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:20:02.17 +14:57:11.5: 15.13 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:16:31.25 +13:38:34.8: 15.01 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.13
Forced photometry filter REJECTED candidate at 01:16:31.25 +13:38:34.8: ref_mag=14.98 +/- 0.13 new_mean_mag=14.7330 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:21:09.29 +13:34:30.2: 15.00 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.14
Forced photometry filter REJECTED candidate at 01:21:09.29 +13:34:30.2: ref_mag=15.19 +/- 0.14 new_mean_mag=14.7298 delta=0.46 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:20:02.17 +14:57:11.5: 14.69 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Forced photometry filter REJECTED candidate at 01:20:02.17 +14:57:11.5: ref_mag=14.87 +/- 0.12 new_mean_mag=14.7523 delta=0.11 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:19:21.54 +14:09:34.7: 15.33 +/- 0.20 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:27:58.38 +16:45:53.8: 15.35 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:19:21.54 +14:09:34.7: 15.53 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.39 +/- 0.17
Forced photometry filter REJECTED candidate at 01:19:21.54 +14:09:34.7: ref_mag=15.39 +/- 0.17 new_mean_mag=14.7809 delta=0.61 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:27:58.38 +16:45:53.8: 15.08 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.13
Forced photometry filter REJECTED candidate at 01:27:58.38 +16:45:53.8: ref_mag=15.21 +/- 0.13 new_mean_mag=14.8781 delta=0.33 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:18:51.42 +10:50:27.5: 15.20 +/- 0.20 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:18:51.42 +10:50:27.5: 14.80 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.13
Forced photometry filter REJECTED candidate at 01:18:51.42 +10:50:27.5: ref_mag=14.97 +/- 0.13 new_mean_mag=14.7008 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 01:24:42.12 +12:47:25.2: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:18:15.80 +12:24:37.0: 15.27 +/- 0.20 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:24:42.12 +12:47:25.2: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:18:15.80 +12:24:37.0: 14.86 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.13
Forced photometry filter REJECTED candidate at 01:18:15.80 +12:24:37.0: ref_mag=15.05 +/- 0.13 new_mean_mag=14.8534 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:38.00 +09:39:02.9: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:41:38.00 +09:39:02.9: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:25.20 +16:56:06.2: 14.85 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:30:25.20 +16:56:06.2: 14.83 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.10
Forced photometry filter REJECTED candidate at 01:30:25.20 +16:56:06.2: ref_mag=14.84 +/- 0.10 new_mean_mag=14.7664 delta=0.08 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:47:03.93 +18:11:46.6: 14.95 +/- 0.12 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:47:03.93 +18:11:46.6: 15.03 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.10
Forced photometry filter REJECTED candidate at 01:47:03.93 +18:11:46.6: ref_mag=14.98 +/- 0.10 new_mean_mag=14.9010 delta=0.08 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:26:37.17 +11:22:08.9: 15.04 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:26:37.17 +11:22:08.9: 15.11 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.12
Forced photometry filter REJECTED candidate at 01:26:37.17 +11:22:08.9: ref_mag=15.07 +/- 0.12 new_mean_mag=14.9601 delta=0.11 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:37:23.83 +14:41:10.2: 15.17 +/- 0.13 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136.fits at 01:37:23.83 +14:41:10.2: 15.40 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.11
Forced photometry filter REJECTED candidate at 01:37:23.83 +14:41:10.2: ref_mag=15.24 +/- 0.11 new_mean_mag=15.0354 delta=0.20 (need > 0.90)
Adding exclusion_list_local.txt__out51084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51699.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 24s
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: 14s
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Considering the candidate 50891_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 50891_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 50899_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 50899_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 50902_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 50902_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:45:28.84 +17:08:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50904_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 50904_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 50905_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 50905_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 50908_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 50908_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:28:36.33 +14:39:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51084_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51084_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51092_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51092_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:32:14.07 +09:13:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51128_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51128_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51135_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51135_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51181_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51181_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51212_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51212_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:55:20.39 +15:20:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51221_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51221_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 02:03:35.94 +18:14:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 51232_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51232_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:33:16.97 +11:57:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51253_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51253_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51309_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51309_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51319_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51319_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51326_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51326_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:39:44.50 +16:26:01.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 51339_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51339_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 02:14:54.07 +08:56:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51342_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51342_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:48:50.93 +16:23:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51435_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51435_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 01:48:36.63 +10:04:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51449_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51449_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 02:01:25.90 +17:58:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51513_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51513_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51524_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51524_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51536_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51536_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51576_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51576_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51589_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51589_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51606_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51606_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51609_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51609_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51638_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51638_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51649_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51649_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51655_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51655_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51676_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51676_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51678_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51678_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51684_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51684_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51690_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51690_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51699_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 51699_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 51717_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51717_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51725_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51725_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51727_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51727_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 51728_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 51728_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 29370_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 29370_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 02:00:56.11 +09:45:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31656_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373
The candidate 31656_fd_Psc-03-Q1b1x1_2026-07-23_04-59-58_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
