This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3
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 27.4186 2461248.9186 7.89 01:42:44.58 +01:46:32.4
148.11172 -58.56527 galactic Cet Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.4 Vesta 0 0 0 7.8 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:42:44.58 +01:46:32.4: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:42:44.58 +01:46:32.4: 16.40 +/- 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 27.4186* 01 42 44.58 +01 46 32.4 7.9 U Cet 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,2461248.9186,7.89,0.05,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 20260727.4186 7.89CV 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 27.4186 2461248.9186 9.60 01:29:29.39 +01:46:08.6
142.03463 -59.68394 galactic Cet Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2 Pallas -0 -0 1 9.5 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:29:29.39 +01:46:08.6: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:29:29.39 +01:46:08.6: 16.33 +/- 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 27.4186* 01 29 29.39 +01 46 08.6 9.6 U Cet 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,2461248.9186,9.60,0.05,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 20260727.4186 9.60CV 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 27.4186 2461248.9186 12.61 01:44:02.52 +10:51:45.7
143.23961 -49.92347 galactic Psc Second-epoch detections are separated by 0.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -0 -0 1 12.6 -0 -0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:44:02.52 +10:51:45.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:44:02.52 +10:51:45.7: 16.59 +/- 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,2461248.9186,12.61,0.05,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 20260727.4186 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4186 2461248.9186 13.20 01:37:12.44 +10:20:01.9
140.96934 -50.92795 galactic Psc Second-epoch detections are separated by 0.4" and 8.1 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 -1 1 13.1 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:37:12.44 +10:20:01.9: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:37:12.44 +10:20:01.9: 16.54 +/- 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,2461248.9186,13.20,0.05,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 20260727.4186 13.20CV 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 27.4186 2461248.9186 13.80 01:37:08.97 +03:50:34.7
144.28783 -57.12126 galactic Psc Second-epoch detections are separated by 0.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.622 Esther -1 -1 1 14.0 -0 -0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:37:08.97 +03:50:34.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:37:08.97 +03:50:34.7: 16.68 +/- 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,2461248.9186,13.80,0.05,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 20260727.4186 13.80CV 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 27.4186 2461248.9186 13.96 01:17:19.80 +03:24:09.9
135.49223 -58.83613 galactic Psc Second-epoch detections are separated by 0.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.191 Kolga -1 0 1 14.0 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:17:19.80 +03:24:09.9: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:17:19.80 +03:24:09.9: 16.32 +/- 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,2461248.9186,13.96,0.05,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 20260727.4186 13.96CV 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 27.4186 2461248.9186 14.01 01:18:22.58 +06:11:16.0
134.98251 -56.05240 galactic Psc Second-epoch detections are separated by 1.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.58 Concordia -1 -1 1 14.2 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:18:22.58 +06:11:16.0: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:18:22.58 +06:11:16.0: 16.51 +/- 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,2461248.9186,14.01,0.05,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 20260727.4186 14.01CV 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
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
PSN J01232438+0925545,2461248.9186,14.34,0.05,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
PSN J01232438+0925545 20260727.4186 14.34CV 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 27.4186 2461248.9186 14.43 01:44:26.01 +09:51:39.4
143.88350 -50.84229 galactic Psc Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.167 Urda 0 0 0 14.7 0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:44:26.01 +09:51:39.4: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:44:26.01 +09:51:39.4: 16.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.9186,14.43,0.05,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 20260727.4186 14.43CV 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 27.4186 2461248.9186 14.46 01:34:53.30 +08:44:29.7
140.79764 -52.61642 galactic Psc Second-epoch detections are separated by 0.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.329 Svea -1 -0 1 14.4 -0 0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:34:53.30 +08:44:29.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:34:53.30 +08:44:29.7: 16.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.9186,14.46,0.05,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 20260727.4186 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4186 2461248.9186 14.58 01:38:11.09 +08:37:53.3
142.13330 -52.48878 galactic Psc Second-epoch detections are separated by 1.5" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1317 Silvretta -1 -1 1 15.0 -0 -0
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:38:11.09 +08:37:53.3: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:38:11.09 +08:37:53.3: 16.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.9186,14.58,0.05,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 20260727.4186 14.58CV 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: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
First image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Last image: 2461248.91889264 27.07.2026 10:03:02.324 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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: 11 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): 6855
Objects passed selection criteria: 6846
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: 7105.5
Average stars matched: 6192.5 (87.1508 %)
Memory usage VmPeak: 233936 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 06:07:41 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: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
First image: 2461049.63853609 09.01.2026 03:19:19.518 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Last image: 2461248.91889264 27.07.2026 10:03:02.324 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 22 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): 35435
Objects passed selection criteria: 35367
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 33473
Average stars matched: 30691.2 (91.6896 %)
Memory usage VmPeak: 259416 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 06:11:24 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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.cat to cache
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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: 2461248.91821882
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits exists and is non-empty
Saving wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits to local_wcs_cache/
'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits' -> 'local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits'
wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits exists and is non-empty
Saving wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits to local_wcs_cache/
'wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits' -> 'local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits'
wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits exists and is non-empty
Saving wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits'
wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits exists and is non-empty
Saving wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits (1st reference image)
verification OK: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:52.021 +05:59:59.08 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-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits (1st new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:43:05.393 +06:00:03.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:43:05.393 +06:00:03.47
Angular distance between the image centers 0.0554 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits (2nd new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:43:08.044 +06:00:33.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:43:08.044 +06:00:33.13
Angular distance between the image centers 0.0671 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 01:43:05.393 +06:00:03.47
Second-epoch second image center 01:43:08.044 +06:00:33.13
Angular distance between the image centers 0.01373 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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits &> /tmp/tmp.dHCuXCQuNl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits &> /tmp/tmp.4KcQuNmq7R
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits &> /tmp/tmp.yeGreK110v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits &> /tmp/tmp.rFnQlE9M4Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat
The reference image (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits) and catalog (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat) found
'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 6596 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7094 to +11.2856 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 17.7260 to 33.6942 deg, Dec 0.7094 to 11.2856 deg
Loaded 4459 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): 3597 out of 3790 total matches.
Matched with Tycho-2 3790 out of 6596 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.907900
a=0.000000 b=1.000000 c=22.907900
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6596 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7094 to +11.2856 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 17.7260 to 33.6942 deg, Dec 0.7094 to 11.2856 deg
Loaded 4459 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): 3597 out of 3790 total matches.
Matched with Tycho-2 3790 out of 6596 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits (aperture=5.9)
Read 10038 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7262 to 33.6942 deg, Dec +0.6961 to +11.2761 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 17.7262 to 33.6942 deg, Dec 0.6961 to 11.2761 deg
Loaded 4458 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): 3599 out of 3871 total matches.
Matched with Tycho-2 3871 out of 10038 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
2.1 pix Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
2.7 pix fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
2.7 pix fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
2.0 pix wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
2.1 pix wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
Limiting magnitude estimates:
15.3 mag. Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
15.8 mag. Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
14.9 mag. fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
14.9 mag. fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
All-image limiting magnitude estimate: 14.9 (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.dHCuXCQuNl (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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=487, bad_region=0, passed=6596
Got 6596 stars (including 6101 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 6596 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6502 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 6503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits N_match=963 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.280 sigma_q3_arcsec=0.265 sigma_q4_arcsec=0.239 n_q1=232 n_q2=240 n_q3=246 n_q4=245 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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.4KcQuNmq7R (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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=711, bad_region=1, passed=10038
Got 10038 stars (including 9317 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 10038 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 453 to 508 (Dec 0.7 to 11.3)
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(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 9897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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(), 9896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 9896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.20"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits (swarp) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits N_match=971 sigma_overall_arcsec=0.208 sigma_q1_arcsec=0.249 sigma_q2_arcsec=0.186 sigma_q3_arcsec=0.203 sigma_q4_arcsec=0.201 n_q1=232 n_q2=245 n_q3=247 n_q4=247 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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.yeGreK110v (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.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=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=320, bad_region=0, passed=5962
Got 5962 stars (including 5635 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat
util/solve_plate_with_UCAC5 got 5962 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 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: 964 matched stars entering correct_measured_positions(), 5920 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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=964 robust_rms=10.113 arcsec
SIP_REFIT: SIP order 3 trial: matched=964 robust_rms=0.324 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=964 robust_rms_before=0.961 arcsec robust_rms_before_corrected=0.252 arcsec robust_rms_after=0.324 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.252 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits N_match=964 sigma_overall_arcsec=0.267 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.293 sigma_q3_arcsec=0.241 sigma_q4_arcsec=0.249 n_q1=242 n_q2=245 n_q3=240 n_q4=237 worst_quadrant_to_overall_ratio=1.096
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits -region wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.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.rFnQlE9M4Z (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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=364, bad_region=0, passed=6006
Got 6006 stars (including 5637 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat
util/solve_plate_with_UCAC5 got 6006 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=965 robust_rms=10.425 arcsec
SIP_REFIT: SIP order 3 trial: matched=965 robust_rms=0.346 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=965 robust_rms_before=0.953 arcsec robust_rms_before_corrected=0.243 arcsec robust_rms_after=0.346 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.243 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits N_match=965 sigma_overall_arcsec=0.257 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.292 sigma_q3_arcsec=0.241 sigma_q4_arcsec=0.216 n_q1=237 n_q2=249 n_q3=244 n_q4=235 worst_quadrant_to_overall_ratio=1.137
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits -region wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits sigma_overall=0.294 worst_q_ratio=1.217
ref2=Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits sigma_overall=0.208 worst_q_ratio=1.196
new1=fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits sigma_overall=0.267 worst_q_ratio=1.096
new2=fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits sigma_overall=0.257 worst_q_ratio=1.137
reference average sigma_overall=0.251 worst_q_ratio=1.2065
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1_astrometric_residuals.png (963 matched stars from wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2_astrometric_residuals.png (971 matched stars from wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.19 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310_astrometric_residuals.png (964 matched stars from wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311_astrometric_residuals.png (965 matched stars from wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits'
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits'
Preparing the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:29:29.39 +01:46:08.6: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:42:44.58 +01:46:32.4: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:29:29.39 +01:46:08.6: 16.33 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:42:44.58 +01:46:32.4: 16.40 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out23445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23460.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23445_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 23445_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23460_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 23460_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01475_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 01475_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:17:34.86 +08:55:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05218_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 05218_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:30:38.37 +02:52:55.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 12s
Prepared the HTML report for the field Psc-06-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 ####
01:42:44.58 +01:46:32.4
01:29:29.39 +01:46:08.6
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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.cat to cache
SExtractor catalog cache: saved Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Creating symlink local_wcs_cache/wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits exists and is non-empty
wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits (1st reference image)
verification OK: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:52.021 +05:59:59.08 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-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits (1st new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:43:05.393 +06:00:03.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:43:05.393 +06:00:03.47
Angular distance between the image centers 0.0554 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits (2nd new image)
verification OK: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:43:08.044 +06:00:33.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:52.021 +05:59:59.08
Second-epoch image center 01:43:08.044 +06:00:33.13
Angular distance between the image centers 0.0671 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 01:43:05.393 +06:00:03.47
Second-epoch second image center 01:43:08.044 +06:00:33.13
Angular distance between the image centers 0.01373 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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits &> /tmp/tmp.FfqPEjWHup
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits &> /tmp/tmp.Z6Pr6UxPrE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits &> /tmp/tmp.HcLfu82d9g
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits &> /tmp/tmp.n2u8YwR1r0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat
Found non-empty wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits and wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat
The reference image (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits) and catalog (wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat) found
'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 34861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7059 to +11.2869 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 17.7260 to 33.6942 deg, Dec 0.7059 to 11.2869 deg
Loaded 4462 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): 3480 out of 3876 total matches.
Matched with Tycho-2 3876 out of 34861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.813150
a=0.000000 b=1.000000 c=22.813150
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7260 to 33.6942 deg, Dec +0.7059 to +11.2869 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 17.7260 to 33.6942 deg, Dec 0.7059 to 11.2869 deg
Loaded 4462 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): 3480 out of 3876 total matches.
Matched with Tycho-2 3876 out of 34861 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits (aperture=4.8)
Read 44485 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.7262 to 33.7121 deg, Dec +0.6960 to +11.2774 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 17.7262 to 33.7121 deg, Dec 0.6960 to 11.2774 deg
Loaded 4462 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): 3346 out of 3874 total matches.
Matched with Tycho-2 3874 out of 44485 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits:
Forced-photometry filter: calibrated wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits -> calib.txt_param_ref_wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
2.1 pix Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
2.6 pix fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
2.6 pix fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
1.9 pix wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
2.1 pix wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
Limiting magnitude estimates:
15.4 mag. Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
15.9 mag. Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
15.0 mag. fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
15.0 mag. fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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.FfqPEjWHup (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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=11, blended=1454, bad_region=1, passed=34850
Got 34850 stars (including 33348 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 34850 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 34391 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 34392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 34392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits N_match=961 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.275 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.260 n_q1=235 n_q2=235 n_q3=240 n_q4=251 worst_quadrant_to_overall_ratio=1.208
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.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.Z6Pr6UxPrE (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits' -> 'wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat corresponding to the image wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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=26, blended=2374, bad_region=2, passed=44459
Got 44459 stars (including 42021 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 44459 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 453 to 508 (Dec 0.7 to 11.3)
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(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 44127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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(), 44128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 44128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits N_match=969 sigma_overall_arcsec=0.212 sigma_q1_arcsec=0.261 sigma_q2_arcsec=0.213 sigma_q3_arcsec=0.197 sigma_q4_arcsec=0.187 n_q1=230 n_q2=243 n_q3=256 n_q4=240 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits -region wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.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.HcLfu82d9g (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.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=7, blended=961, bad_region=14, passed=27780
Got 27780 stars (including 26768 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat
util/solve_plate_with_UCAC5 got 27780 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 27579 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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 27581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 27581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits N_match=962 sigma_overall_arcsec=0.264 sigma_q1_arcsec=0.270 sigma_q2_arcsec=0.283 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.252 n_q1=244 n_q2=241 n_q3=234 n_q4=243 worst_quadrant_to_overall_ratio=1.075
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits -region wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.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.n2u8YwR1r0 (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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=917, bad_region=20, passed=27645
Got 27645 stars (including 26672 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat
util/solve_plate_with_UCAC5 got 27645 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 27496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 27495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 27495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits N_match=963 sigma_overall_arcsec=0.257 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.233 sigma_q4_arcsec=0.216 n_q1=241 n_q2=244 n_q3=240 n_q4=238 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits -region wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-02-04_20.00sec_-0.00C_LIGHTs_0310.fits
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.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_2026-07-27_CI_Psc-06-Q1b1x1_051728_TTUQ1b1x1_727255_LrKx3Gw3/wcs_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311.fits
Preparing the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:28:54.60 +06:33:02.9: 13.23 +/- 0.03 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:37:12.44 +10:20:01.9: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:19:55.54 +02:43:02.1: 13.42 +/- 0.04 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:34:31.11 +05:38:56.0: 14.17 +/- 0.06 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:21:29.94 +03:46:27.6: 12.87 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:31:07.03 +07:42:04.1: 12.75 +/- 0.02 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:44:02.52 +10:51:45.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:37:12.44 +10:20:01.9: 16.54 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:19:55.54 +02:43:02.1: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter REJECTED candidate at 01:19:55.54 +02:43:02.1: ref_mag=13.31 +/- 0.02 new_mean_mag=13.3779 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:34:31.11 +05:38:56.0: 14.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.03
Forced photometry filter REJECTED candidate at 01:34:31.11 +05:38:56.0: ref_mag=14.04 +/- 0.03 new_mean_mag=14.2829 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:44:02.52 +10:51:45.7: 16.59 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:28:54.60 +06:33:02.9: 13.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.01
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:53:17.14 +07:00:52.7: 13.74 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 01:28:54.60 +06:33:02.9: ref_mag=13.18 +/- 0.01 new_mean_mag=13.3816 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:37:08.97 +03:50:34.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:23:49.78 +06:29:04.4: 13.85 +/- 0.05 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:21:29.94 +03:46:27.6: 12.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter REJECTED candidate at 01:21:29.94 +03:46:27.6: ref_mag=12.79 +/- 0.01 new_mean_mag=13.0600 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:31:07.03 +07:42:04.1: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter REJECTED candidate at 01:31:07.03 +07:42:04.1: ref_mag=12.68 +/- 0.01 new_mean_mag=12.8800 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:53:17.14 +07:00:52.7: 13.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Forced photometry filter REJECTED candidate at 01:53:17.14 +07:00:52.7: ref_mag=13.65 +/- 0.02 new_mean_mag=13.6248 delta=0.02 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:23:49.78 +06:29:04.4: 13.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter REJECTED candidate at 01:23:49.78 +06:29:04.4: ref_mag=13.74 +/- 0.03 new_mean_mag=13.6942 delta=0.04 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:37:08.97 +03:50:34.7: 16.68 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:17:19.80 +03:24:09.9: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:18:22.58 +06:11:16.0: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:44:31.09 +10:55:37.7: 13.97 +/- 0.06 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:43:02.70 +07:09:27.1: 14.16 +/- 0.06 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:18:22.58 +06:11:16.0: 16.51 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:30:22.34 +11:04:37.6: 14.30 +/- 0.09 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:17:19.80 +03:24:09.9: 16.32 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:44:26.01 +09:51:39.4: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:44:31.09 +10:55:37.7: 13.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.03
Forced photometry filter REJECTED candidate at 01:44:31.09 +10:55:37.7: ref_mag=13.92 +/- 0.03 new_mean_mag=14.0027 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:30:22.34 +11:04:37.6: 14.35 +/- 0.06 detection
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:43:02.70 +07:09:27.1: 14.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.05
Forced photometry filter REJECTED candidate at 01:30:22.34 +11:04:37.6: ref_mag=14.34 +/- 0.05 new_mean_mag=14.2281 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.18 +/- 0.03
Forced photometry filter REJECTED candidate at 01:43:02.70 +07:09:27.1: ref_mag=14.18 +/- 0.03 new_mean_mag=14.2316 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:44:26.01 +09:51:39.4: 16.60 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:34:53.30 +08:44:29.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091_stack1.fits at 01:38:11.09 +08:37:53.3: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:34:53.30 +08:44:29.7: 16.61 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_stack2.fits at 01:38:11.09 +08:37:53.3: 16.66 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out60111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60801.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 11s
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Considering the candidate 59924_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 59924_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 59929_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 59929_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 59930_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 59930_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 59932_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 59932_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 59935_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 59935_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:42:44.57 +01:46:32.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 59951_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 59951_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:29:29.39 +01:46:08.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 60102_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60102_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:32:14.11 +09:13:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60111_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60111_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60170_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60170_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 60220_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60220_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60331_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60331_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 60343_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60343_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 60400_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60400_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60418_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60418_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60419_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60419_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:36:55.65 +08:52:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60457_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60457_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:31:14.72 +08:48:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60462_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60462_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60465_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60465_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 60601_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60601_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 60606_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 60606_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
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Considering the candidate 60631_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60631_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60758_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60758_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60772_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60772_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 60801_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
Preparing report for the candidate 60801_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
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Considering the candidate 07477_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 07477_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
**** FOUND 01:17:34.86 +08:55:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29199_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311
The candidate 29199_fd_Psc-06-Q1b1x1_2026-07-27_05-03-02_20.00sec_-0.00C_LIGHTs_0311 did not pass the final checks
