This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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,2461286.9571,8.15,0.05,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 20260903.4571 8.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 11.55 00:07:08.61 -06:25:53.5
93.97859 -66.78004 galactic Cet Second-epoch detections are separated by 0.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.106 Dione -0 1 1 11.8 0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:07:08.61 -06:25:53.5: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:07:08.61 -06:25:53.5: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 03.4571* 00 07 08.61 -06 25 53.5 11.6 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,2461286.9571,11.55,0.05,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 20260903.4571 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 12.35 23:59:10.07 -01:16:34.0
94.88267 -61.26840 galactic Psc Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.317 Roxane -1 0 1 12.2 -0 -0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:59:10.07 -01:16:34.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:59:10.07 -01:16:34.0: 15.79 +/- 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,2461286.9571,12.35,0.05,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 20260903.4571 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 12.39 00:16:33.38 -01:53:48.8
103.13697 -63.42009 galactic Psc Second-epoch detections are separated by 0.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.217 Eudora 0 0 0 12.4 0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:16:33.38 -01:53:48.8: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:16:33.38 -01:53:48.8: 15.76 +/- 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,2461286.9571,12.39,0.05,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 20260903.4571 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 13.30 23:41:54.51 +00:20:36.3
88.78648 -57.84335 galactic Psc Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.570 Kythera -0 -0 0 13.3 0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:41:54.51 +00:20:36.3: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:41:54.51 +00:20:36.3: 15.63 +/- 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,2461286.9571,13.30,0.05,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 20260903.4571 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 13.34 23:37:05.13 +00:19:08.2
86.83310 -57.24694 galactic Psc Second-epoch detections are separated by 0.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.788 Hohensteina -0 -1 1 13.6 -0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:37:05.13 +00:19:08.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:37:05.13 +00:19:08.2: 15.64 +/- 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,2461286.9571,13.34,0.05,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
VARIABLE_NAME 20260903.4571 13.34CV 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 09 03.4571 2461286.9571 13.36 23:48:00.82 -01:23:32.5
89.69891 -60.10637 galactic Psc Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.328 Gudrun 0 0 0 13.6 0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:48:00.82 -01:23:32.5: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:48:00.82 -01:23:32.5: 15.78 +/- 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,2461286.9571,13.36,0.05,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 20260903.4571 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 13.84 00:24:03.49 +02:30:40.6
109.30861 -59.63431 galactic Psc Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.551 Ortrud 0 0 0 14.1 -0 -0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:24:03.49 +02:30:40.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:24:03.49 +02:30:40.6: 15.67 +/- 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,2461286.9571,13.84,0.05,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 20260903.4571 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 13.74 23:46:56.09 -02:15:51.0
88.34773 -60.72912 galactic Psc Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.799 Gudula 0 0 0 13.6 -0 -0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:46:56.09 -02:15:51.0: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:46:56.09 -02:15:51.0: 15.76 +/- 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,2461286.9571,13.74,0.05,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 20260903.4571 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 14.10 23:39:04.78 +01:43:13.1
88.92242 -56.29729 galactic Psc Second-epoch detections are separated by 1.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.673 Edda -0 0 1 14.2 -0 -0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:39:04.78 +01:43:13.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:39:04.78 +01:43:13.1: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461286.9571,14.10,0.05,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 20260903.4571 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.4571 2461286.9571 11.96 23:51:14.94 -02:45:49.9
89.77491 -61.69790 galactic Psc Second-epoch detections are separated by 0.4" and 5.5 pix
The object was found in VSX 1" ASAS J235115-0245.8
Type: SRA
# Max. Min./Amp. JD0 Period
12.000 V 14.000 V 2454301.00000 132.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:51:14.94 -02:45:49.9: 12.90 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:51:14.94 -02:45:49.9: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
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
ASAS J235115-0245.8,2461286.9571,11.96,0.05,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
ASAS J235115-0245.8 20260903.4571 11.96CV 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
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,2461286.9571,8.26,0.05,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 20260903.4571 8.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
First image: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Last image: 2461286.95739282 03.09.2026 10:58:28.740 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.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.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5288
Objects passed selection criteria: 5277
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 4201
Average stars matched: 4097.5 (97.5363 %)
Memory usage VmPeak: 231796 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 06:41:50 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: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
First image: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Last image: 2461286.95739282 03.09.2026 10:58:28.740 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 10 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 27900
Objects passed selection criteria: 27820
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 24673.5
Average stars matched: 23690.8 (96.017 %)
Memory usage VmPeak: 251732 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 06:42:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
SExtractor catalog cache: saved Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.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: 2461286.95684875
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits exists and is non-empty
wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits exists and is non-empty
wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits exists and is non-empty
wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (1st reference image)
verification OK: wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.424 -02:00:17.62 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:41.383 -01:59:28.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 23:59:41.383 -01:59:28.21
Angular distance between the image centers 0.0805 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Image size: 941.6'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:42.042 -01:58:56.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 23:59:42.042 -01:58:56.14
Angular distance between the image centers 0.0798 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:41.383 -01:59:28.21
Second-epoch second image center 23:59:42.042 -01:58:56.14
Angular distance between the image centers 0.00932 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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits &> /tmp/tmp.CXI7G9ewLi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits &> /tmp/tmp.aYoEQGHi9X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits &> /tmp/tmp.L2IG40QghS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits &> /tmp/tmp.WhZsPvX4Ia
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
Found non-empty wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
The reference image (wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits) and catalog (wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat) found
'wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 5537 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1391 to 7.8851 deg, Dec -7.2685 to +3.2742 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 352.1391 to 7.8851 deg, Dec -7.2685 to 3.2742 deg
Loaded 113496 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): 3358 out of 3443 total matches.
Matched with Tycho-2 3443 out of 5537 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.638200
a=0.000000 b=1.000000 c=22.638200
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 5537 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1391 to 7.8851 deg, Dec -7.2685 to +3.2742 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 352.1391 to 7.8851 deg, Dec -7.2685 to 3.2742 deg
Loaded 113496 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): 3358 out of 3443 total matches.
Matched with Tycho-2 3443 out of 5537 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -> calib.txt_param_ref_wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (aperture=6.4)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 5464 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1355 to 7.8705 deg, Dec -7.2684 to +3.2771 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 352.1355 to 7.8705 deg, Dec -7.2684 to 3.2771 deg
Loaded 113493 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): 3322 out of 3420 total matches.
Matched with Tycho-2 3420 out of 5464 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -> calib.txt_param_ref_wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (aperture=6.3)
____ 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:
2.3 pix Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
2.2 pix Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
2.1 pix fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
2.2 pix fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Limiting magnitude estimates:
15.0 mag. Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
15.0 mag. Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
14.3 mag. fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
14.3 mag. fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.CXI7G9ewLi (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits' -> 'wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS-calibrated image found: wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Checking if the catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS catalog name: wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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=342, bad_region=0, passed=5537
Got 5537 stars (including 5189 good ones) from the SExtractor catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
util/solve_plate_with_UCAC5 got 5537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1391 through 0 to 7.8851, gap 7.8851 to 352.1391
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 5537 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
RA wraps around 0/360 boundary: field RA 352.1393 through 0 to 7.8849, gap 7.8849 to 352.1393
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 5537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 5537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4890 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits N_match=4890 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.349 sigma_q4_arcsec=0.323 n_q1=1237 n_q2=1170 n_q3=1280 n_q4=1203 worst_quadrant_to_overall_ratio=1.085
The image catalog is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -region wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.aYoEQGHi9X (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits' -> 'wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS-calibrated image found: wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Checking if the catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS catalog name: wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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=354, bad_region=0, passed=5461
Got 5461 stars (including 5101 good ones) from the SExtractor catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat
util/solve_plate_with_UCAC5 got 5461 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1355 through 0 to 7.8705, gap 7.8705 to 352.1355
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 4884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 5461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1357 through 0 to 7.8704, gap 7.8704 to 352.1357
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 5461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 5461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4883 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits N_match=4883 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.387 sigma_q3_arcsec=0.407 sigma_q4_arcsec=0.354 n_q1=1244 n_q2=1180 n_q3=1267 n_q4=1192 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -region wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.L2IG40QghS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.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=254, bad_region=0, passed=2966
Got 2966 stars (including 2709 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat
util/solve_plate_with_UCAC5 got 2966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7913 through 0 to 8.0632, gap 8.0632 to 351.7913
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 2646 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2644 matched stars entering correct_measured_positions(), 2644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2644 matched stars entering correct_measured_positions(), 2966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7912 through 0 to 8.0637, gap 8.0637 to 351.7912
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 2646 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2644 matched stars entering correct_measured_positions(), 2966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 2644 matched stars entering correct_measured_positions(), 2966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 2644 stars left (next iteration limit 2908)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2644 robust_rms=10.937 arcsec worst_quadrant_rms=11.753 arcsec
SIP_REFIT: SIP order 3 trial: matched=2644 robust_rms=0.513 arcsec worst_quadrant_rms=0.572 arcsec
SIP_REFIT: SIP order 5 trial: matched=2644 robust_rms=0.321 arcsec worst_quadrant_rms=0.362 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2644 robust_rms_before=1.010 arcsec robust_rms_before_corrected=0.330 arcsec robust_rms_after=0.321 arcsec worst_quadrant_rms_before=0.388 worst_quadrant_rms_after=0.362
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.388 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits N_match=2644 sigma_overall_arcsec=0.332 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.376 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.303 n_q1=642 n_q2=676 n_q3=650 n_q4=676 worst_quadrant_to_overall_ratio=1.134
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.WhZsPvX4Ia (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.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=259, bad_region=0, passed=2971
Got 2971 stars (including 2707 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat
util/solve_plate_with_UCAC5 got 2971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
RA wraps around 0/360 boundary: field RA 351.7913 through 0 to 8.0631, gap 8.0631 to 351.7913
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 2647 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2645 matched stars entering correct_measured_positions(), 2645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2645 matched stars entering correct_measured_positions(), 2971 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
RA wraps around 0/360 boundary: field RA 351.7912 through 0 to 8.0638, gap 8.0638 to 351.7912
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 2647 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2645 matched stars entering correct_measured_positions(), 2971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 2645 matched stars entering correct_measured_positions(), 2971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 2645 stars left (next iteration limit 2909)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2645 robust_rms=10.397 arcsec worst_quadrant_rms=11.383 arcsec
SIP_REFIT: SIP order 3 trial: matched=2645 robust_rms=0.543 arcsec worst_quadrant_rms=0.593 arcsec
SIP_REFIT: SIP order 5 trial: matched=2645 robust_rms=0.352 arcsec worst_quadrant_rms=0.391 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2645 robust_rms_before=1.037 arcsec robust_rms_before_corrected=0.348 arcsec robust_rms_after=0.352 arcsec worst_quadrant_rms_before=0.390 worst_quadrant_rms_after=0.391
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.390 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits N_match=2645 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.323 n_q1=637 n_q2=684 n_q3=647 n_q4=677 worst_quadrant_to_overall_ratio=1.113
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits to local_wcs_cache/
'wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits' -> 'local_wcs_cache/wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits'
Saving the final (post-refit) wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits to local_wcs_cache/
'wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits' -> 'local_wcs_cache/wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits'
Saving the final (post-refit) wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits'
Saving the final (post-refit) wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits sigma_overall=0.322 worst_q_ratio=1.085
ref2=Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits sigma_overall=0.364 worst_q_ratio=1.116
new1=fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits sigma_overall=0.332 worst_q_ratio=1.134
new2=fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits sigma_overall=0.356 worst_q_ratio=1.113
reference average sigma_overall=0.343 worst_q_ratio=1.1005
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999_astrometric_residuals.png (4890 matched stars from wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000_astrometric_residuals.png (4883 matched stars from wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475_astrometric_residuals.png (2644 matched stars from wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476_astrometric_residuals.png (2645 matched stars from wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits'
Saving fully-calibrated image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits'
Preparing the HTML report for the field Psc-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:26:53.01 -05:30:58.5: 10.01 +/- 0.00 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:07:08.61 -06:25:53.5: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:26:53.01 -05:30:58.5: 10.07 +/- 0.00 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:07:08.61 -06:25:53.5: 15.56 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.04 +/- 0.00
Forced photometry filter REJECTED candidate at 00:26:53.01 -05:30:58.5: ref_mag=10.04 +/- 0.00 new_mean_mag=10.1350 delta=-0.10 (need > 0.90)
Adding exclusion_list_local.txt__out20391.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20269_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 20269_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 20275_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 20275_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20391_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 20391_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03946_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 03946_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
**** FOUND 23:44:04.79 +00:22:53.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Psc-08-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 ####
00:07:08.61 -06:25:53.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
SExtractor catalog cache: saved Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Creating symlink local_wcs_cache/wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits exists and is non-empty
wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits exists and is non-empty
wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits exists and is non-empty
wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (1st reference image)
verification OK: wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.424 -02:00:17.62 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:41.383 -01:59:28.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 23:59:41.383 -01:59:28.21
Angular distance between the image centers 0.0805 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Image size: 941.6'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:42.042 -01:58:56.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 23:59:42.042 -01:58:56.14
Angular distance between the image centers 0.0798 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:41.383 -01:59:28.21
Second-epoch second image center 23:59:42.042 -01:58:56.14
Angular distance between the image centers 0.00932 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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits &> /tmp/tmp.R62zB9LY6o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits &> /tmp/tmp.tVmopFK84z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits &> /tmp/tmp.AQa0hCoKCq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits &> /tmp/tmp.MkuyZsb0NT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
Found non-empty wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
The reference image (wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits) and catalog (wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat) found
'wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 29281 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1384 to 7.8963 deg, Dec -7.2757 to +3.2741 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 352.1384 to 7.8963 deg, Dec -7.2757 to 3.2741 deg
Loaded 113505 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): 3329 out of 3554 total matches.
Matched with Tycho-2 3554 out of 29281 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.536200
a=0.000000 b=1.000000 c=22.536200
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 29281 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1384 to 7.8963 deg, Dec -7.2757 to +3.2741 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 352.1384 to 7.8963 deg, Dec -7.2757 to 3.2741 deg
Loaded 113505 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): 3329 out of 3554 total matches.
Matched with Tycho-2 3554 out of 29281 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -> calib.txt_param_ref_wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (aperture=5.1)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 30046 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1258 to 7.8769 deg, Dec -7.2751 to +3.2772 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 352.1258 to 7.8769 deg, Dec -7.2751 to 3.2772 deg
Loaded 113502 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): 3314 out of 3546 total matches.
Matched with Tycho-2 3546 out of 30046 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -> calib.txt_param_ref_wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 31 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
2.1 pix Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
2.0 pix fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
2.0 pix fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Limiting magnitude estimates:
15.1 mag. Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
15.2 mag. Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
14.4 mag. fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
14.4 mag. fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.9 (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.R62zB9LY6o (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits' -> 'wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS-calibrated image found: wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Checking if the catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS catalog name: wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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=15, blended=1084, bad_region=0, passed=29266
Got 29266 stars (including 28140 good ones) from the SExtractor catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
util/solve_plate_with_UCAC5 got 29266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1384 through 0 to 7.8963, gap 7.8963 to 352.1384
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 29266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1387 through 0 to 7.8962, gap 7.8962 to 352.1387
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 29266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 29266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4882 stars left (next iteration limit 5370)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits N_match=4882 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.264 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.318 n_q1=1251 n_q2=1169 n_q3=1235 n_q4=1227 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -region wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tVmopFK84z (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits' -> 'wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS-calibrated image found: wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Checking if the catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS catalog name: wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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=15, blended=1265, bad_region=0, passed=30031
Got 30031 stars (including 28725 good ones) from the SExtractor catalog wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat
util/solve_plate_with_UCAC5 got 30031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1258 through 0 to 7.8769, gap 7.8769 to 352.1258
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 4877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 30031 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
RA wraps around 0/360 boundary: field RA 352.1262 through 0 to 7.8768, gap 7.8768 to 352.1262
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 30031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 30031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4877 stars left (next iteration limit 5364)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits N_match=4877 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.345 n_q1=1251 n_q2=1175 n_q3=1234 n_q4=1217 worst_quadrant_to_overall_ratio=1.133
The image catalog is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -region wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.AQa0hCoKCq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.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=14, blended=584, bad_region=16, passed=20143
Got 20143 stars (including 19504 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat
util/solve_plate_with_UCAC5 got 20143 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7395 through 0 to 8.0665, gap 8.0665 to 351.7395
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 4876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 20143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7392 through 0 to 8.0672, gap 8.0672 to 351.7392
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 20143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 20143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4876 stars left (next iteration limit 5363)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4876 robust_rms=10.184 arcsec worst_quadrant_rms=10.592 arcsec
SIP_REFIT: SIP order 3 trial: matched=4876 robust_rms=0.545 arcsec worst_quadrant_rms=0.599 arcsec
SIP_REFIT: SIP order 5 trial: matched=4876 robust_rms=0.364 arcsec worst_quadrant_rms=0.401 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4876 robust_rms_before=1.025 arcsec robust_rms_before_corrected=0.358 arcsec robust_rms_after=0.364 arcsec worst_quadrant_rms_before=0.402 worst_quadrant_rms_after=0.401
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.402 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits N_match=4876 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.366 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.317 n_q1=1250 n_q2=1261 n_q3=1164 n_q4=1201 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.MkuyZsb0NT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.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=5, blended=579, bad_region=18, passed=20046
Got 20046 stars (including 19402 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat
util/solve_plate_with_UCAC5 got 20046 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
RA wraps around 0/360 boundary: field RA 351.7399 through 0 to 8.0666, gap 8.0666 to 351.7399
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 20046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7395 through 0 to 8.0673, gap 8.0673 to 351.7395
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 20046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 20046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4873 robust_rms=10.202 arcsec worst_quadrant_rms=10.478 arcsec
SIP_REFIT: SIP order 3 trial: matched=4873 robust_rms=0.582 arcsec worst_quadrant_rms=0.630 arcsec
SIP_REFIT: SIP order 5 trial: matched=4873 robust_rms=0.395 arcsec worst_quadrant_rms=0.426 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4873 robust_rms_before=1.050 arcsec robust_rms_before_corrected=0.384 arcsec robust_rms_after=0.395 arcsec worst_quadrant_rms_before=0.435 worst_quadrant_rms_after=0.426
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.435 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits N_match=4873 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.417 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.341 n_q1=1256 n_q2=1264 n_q3=1160 n_q4=1193 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Saving fully-calibrated image wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Psc-08-Q1b1x1_063622_TTUQ1b1x1_3901450_RgJ0vZn0/wcs_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476.fits
Preparing the HTML report for the field Psc-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:49:56.15 +01:54:08.4: 12.64 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:44:30.92 -04:38:51.9: 13.26 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:54:09.55 +02:19:04.0: 12.18 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:16:33.38 -01:53:48.8: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:28:30.90 -04:35:30.5: 13.36 +/- 0.05 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:59:10.07 -01:16:34.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:26:53.02 -05:30:58.4: 10.24 +/- 0.00 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:40:03.03 +02:51:52.5: 12.08 +/- 0.01 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:22:25.96 -05:03:57.1: 13.01 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:59:45.74 -05:52:34.0: 12.36 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:49:56.15 +01:54:08.4: 12.67 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:59:10.07 -01:16:34.0: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:40:03.03 +02:51:52.5: 12.06 +/- 0.01 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:54:09.55 +02:19:04.0: 12.19 +/- 0.01 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:28:30.90 -04:35:30.5: 13.43 +/- 0.05 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:22:25.96 -05:03:57.1: 13.06 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:44:30.92 -04:38:51.9: 13.14 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:16:33.38 -01:53:48.8: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:26:53.02 -05:30:58.4: 10.29 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter REJECTED candidate at 23:49:56.15 +01:54:08.4: ref_mag=12.66 +/- 0.02 new_mean_mag=13.0167 delta=-0.36 (need > 0.90)
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry reference-image weighted average: 10.26 +/- 0.00
Forced photometry filter REJECTED candidate at 23:40:03.03 +02:51:52.5: ref_mag=12.07 +/- 0.01 new_mean_mag=12.2623 delta=-0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:54:09.55 +02:19:04.0: ref_mag=12.18 +/- 0.01 new_mean_mag=12.4898 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:28:30.90 -04:35:30.5: ref_mag=13.39 +/- 0.03 new_mean_mag=13.3606 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:22:25.96 -05:03:57.1: ref_mag=13.03 +/- 0.02 new_mean_mag=13.4320 delta=-0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:44:30.92 -04:38:51.9: ref_mag=13.19 +/- 0.03 new_mean_mag=13.7152 delta=-0.52 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:26:53.02 -05:30:58.4: ref_mag=10.26 +/- 0.00 new_mean_mag=10.2158 delta=0.05 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:59:45.74 -05:52:34.0: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter REJECTED candidate at 23:59:45.74 -05:52:34.0: ref_mag=12.37 +/- 0.01 new_mean_mag=12.4485 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:47:44.00 +02:02:26.8: 13.22 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:37:05.13 +00:19:08.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:38:24.47 +01:55:17.0: 12.44 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:45:11.96 +02:18:07.2: 12.41 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:41:54.51 +00:20:36.3: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:48:00.82 -01:23:32.5: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:24:03.49 +02:30:40.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:47:44.00 +02:02:26.8: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter REJECTED candidate at 23:47:44.00 +02:02:26.8: ref_mag=13.24 +/- 0.03 new_mean_mag=13.3025 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:38:24.47 +01:55:17.0: 12.44 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:45:11.96 +02:18:07.2: 12.50 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:37:05.13 +00:19:08.2: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:41:54.51 +00:20:36.3: 15.63 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 23:38:24.47 +01:55:17.0: ref_mag=12.44 +/- 0.01 new_mean_mag=12.6090 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:45:11.96 +02:18:07.2: ref_mag=12.45 +/- 0.01 new_mean_mag=12.5569 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:48:00.82 -01:23:32.5: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:56:27.66 -00:35:54.1: 13.37 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:24:03.49 +02:30:40.6: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:56:27.66 -00:35:54.1: 13.45 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:50:15.86 +01:49:07.0: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter REJECTED candidate at 23:56:27.66 -00:35:54.1: ref_mag=13.41 +/- 0.03 new_mean_mag=13.7043 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:46:56.09 -02:15:51.0: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:39:04.78 +01:43:13.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:50:15.86 +01:49:07.0: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter REJECTED candidate at 23:50:15.86 +01:49:07.0: ref_mag=13.24 +/- 0.03 new_mean_mag=13.6038 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:46:56.09 -02:15:51.0: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:00:36.92 +00:12:02.4: 14.19 +/- 0.11 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:39:04.78 +01:43:13.1: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:00:36.92 +00:12:02.4: 13.97 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Forced photometry filter REJECTED candidate at 00:00:36.92 +00:12:02.4: ref_mag=14.06 +/- 0.07 new_mean_mag=14.3562 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:55:27.87 +01:40:47.1: 14.41 +/- 0.11 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:55:27.87 +01:40:47.1: 14.51 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.09
Forced photometry filter REJECTED candidate at 23:55:27.87 +01:40:47.1: ref_mag=14.45 +/- 0.09 new_mean_mag=14.3895 delta=0.06 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:51:14.94 -02:45:49.9: 12.90 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:51:14.94 -02:45:49.9: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter KEPT candidate at 23:51:14.94 -02:45:49.9: ref_mag=12.89 +/- 0.02 new_mean_mag=11.9602 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out12026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33602.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 32786_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 32786_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 32789_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 32789_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 32790_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 32790_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 32791_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 32791_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 32793_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 32793_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 32795_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 32795_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 32917_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 32917_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
**** FOUND 00:07:08.61 -06:25:53.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 33007_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33007_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33018_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33018_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33023_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33023_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33047_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33047_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33055_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33055_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33067_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33067_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33095_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33095_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
**** FOUND 23:29:32.40 -01:46:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33108_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33108_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
**** FOUND 23:54:52.12 +00:04:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33255_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33255_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33274_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33274_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33295_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33295_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33306_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33306_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33366_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33366_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
**** FOUND 00:17:51.85 +00:22:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33406_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33406_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33431_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33431_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33434_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33434_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33451_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33451_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33579_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33579_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 33602_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 33602_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 33673_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33673_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 33702_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 33702_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
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Considering the candidate 12026_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 12026_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 27938_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
Preparing report for the candidate 27938_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
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Considering the candidate 26990_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476
The candidate 26990_fd_Psc-08-Q1b1x1_2026-09-03_05-58-28_20.00sec_-0.00C_LIGHTs_0476 did not pass the final checks
