This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU
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,2461284.8895,8.21,0.05,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 20260901.3895 8.21CV 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,2461284.8895,8.30,0.05,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 20260901.3895 8.30CV 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 01.3895 2461284.8895 11.53 00:08:22.35 -06:16:58.6
94.83981 -66.77630 galactic Psc Second-epoch detections are separated by 0.8" and 6.5 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 0 0 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 00:08:22.35 -06:16:58.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:08:22.35 -06:16:58.6: 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,2461284.8895,11.53,0.05,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 20260901.3895 11.53CV 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 01.3895 2461284.8895 12.44 00:17:21.00 -01:30:27.1
103.81465 -63.10706 galactic Psc Second-epoch detections are separated by 1.1" and 6.5 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 00:17:21.00 -01:30:27.1: 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 00:17:21.00 -01:30:27.1: 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,2461284.8895,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260901.3895 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 01.3895 2461284.8895 12.76 00:00:37.84 -01:04:07.7
95.75294 -61.23042 galactic Psc Second-epoch detections are separated by 1.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.317 Roxane -0 0 0 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 00:00:37.84 -01:04:07.7: 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 00:00:37.84 -01:04:07.7: 15.83 +/- 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,2461284.8895,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260901.3895 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 01.3895 2461284.8895 13.38 23:43:10.53 +00:29:00.8
89.43420 -57.87853 galactic Psc Second-epoch detections are separated by 0.9" and 6.5 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 13.4 0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:43:10.53 +00:29:00.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:43:10.53 +00:29:00.8: 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,2461284.8895,13.38,0.05,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 20260901.3895 13.38CV 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 01.3895 2461284.8895 13.44 23:38:22.52 +00:34:20.5
87.58522 -57.19799 galactic Psc Second-epoch detections are separated by 0.8" and 6.6 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 -0 0 13.7 -0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:38:22.52 +00:34:20.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:38:22.52 +00:34:20.5: 15.70 +/- 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,2461284.8895,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260901.3895 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 01.3895 2461284.8895 13.52 23:49:39.37 -01:22:05.8
90.44547 -60.28357 galactic Psc Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.328 Gudrun -1 1 1 13.7 0 0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:49:39.37 -01:22:05.8: 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 23:49:39.37 -01:22:05.8: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461284.8895,13.52,0.05,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 20260901.3895 13.52CV 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 01.3895 2461284.8895 13.89 23:48:23.45 -02:01:04.7
89.24332 -60.69767 galactic Psc Second-epoch detections are separated by 3.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.799 Gudula -1 0 1 13.7 -0 -0
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:48:23.45 -02:01:04.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:48:23.45 -02:01:04.7: 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,2461284.8895,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260901.3895 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461284.88992935 01.09.2026 09:21:19.896 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 2 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): 5249
Objects passed selection criteria: 5230
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 3826.5
Average stars matched: 3732.75 (97.55 %)
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 Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 04:26:00 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: 2461284.88992935 01.09.2026 09:21:19.896 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 27
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: 7 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): 27621
Objects passed selection criteria: 27543
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: 22550.5
Average stars matched: 21656 (96.0333 %)
Memory usage VmPeak: 251728 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 04:26:40 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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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: 2461284.88914749
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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits exists and is non-empty
wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Image size: 941.4'x626.8' 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: 23:59:57.600 -02:00:49.56 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 23:59:57.600 -02:00:49.56
Angular distance between the image centers 0.0147 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
Image size: 941.4'x626.8' 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: 23:59:54.990 -02:00:49.45 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 23:59:54.990 -02:00:49.45
Angular distance between the image centers 0.0243 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 23:59:57.600 -02:00:49.56
Second-epoch second image center 23:59:54.990 -02:00:49.45
Angular distance between the image centers 0.01087 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.5VoDWU7sFH
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.bolx1w0PRz
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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits &> /tmp/tmp.WptDmbO2JJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits &> /tmp/tmp.ge8ss51F7R
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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 3 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
2.2 pix fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
2.2 pix fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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
13.9 mag. fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
13.9 mag. fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 10.9 (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.5VoDWU7sFH (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/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.bolx1w0PRz (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/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.WptDmbO2JJ (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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=281, bad_region=0, passed=2229
Got 2229 stars (including 1948 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat
util/solve_plate_with_UCAC5 got 2229 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8565 through 0 to 8.1066, gap 8.1066 to 351.8565
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 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 1894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1892 matched stars entering correct_measured_positions(), 1891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1892 matched stars entering correct_measured_positions(), 2227 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 351.8563 through 0 to 8.1070, gap 8.1070 to 351.8563
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 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 1895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1893 matched stars entering correct_measured_positions(), 2228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 1893 matched stars entering correct_measured_positions(), 2228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 1893 stars left (next iteration limit 2081)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1893 robust_rms=10.219 arcsec worst_quadrant_rms=12.130 arcsec
SIP_REFIT: SIP order 3 trial: matched=1893 robust_rms=0.483 arcsec worst_quadrant_rms=0.539 arcsec
SIP_REFIT: SIP order 5 trial: matched=1893 robust_rms=0.343 arcsec worst_quadrant_rms=0.384 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1893 robust_rms_before=1.021 arcsec robust_rms_before_corrected=0.362 arcsec robust_rms_after=0.343 arcsec worst_quadrant_rms_before=0.400 worst_quadrant_rms_after=0.384
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.400 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits N_match=1893 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.366 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.352 n_q1=443 n_q2=490 n_q3=453 n_q4=507 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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.ge8ss51F7R (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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=269, bad_region=0, passed=2199
Got 2199 stars (including 1930 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat
util/solve_plate_with_UCAC5 got 2199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8567 through 0 to 8.1065, gap 8.1065 to 351.8567
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 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 1878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1877 matched stars entering correct_measured_positions(), 1877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1877 matched stars entering correct_measured_positions(), 2198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8564 through 0 to 8.1070, gap 8.1070 to 351.8564
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 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 1878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1877 matched stars entering correct_measured_positions(), 2197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 1877 matched stars entering correct_measured_positions(), 2197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 1877 stars left (next iteration limit 2064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1877 robust_rms=10.027 arcsec worst_quadrant_rms=11.641 arcsec
SIP_REFIT: SIP order 3 trial: matched=1877 robust_rms=0.502 arcsec worst_quadrant_rms=0.527 arcsec
SIP_REFIT: SIP order 5 trial: matched=1877 robust_rms=0.345 arcsec worst_quadrant_rms=0.375 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1877 robust_rms_before=1.024 arcsec robust_rms_before_corrected=0.361 arcsec robust_rms_after=0.345 arcsec worst_quadrant_rms_before=0.415 worst_quadrant_rms_after=0.375
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.415 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits N_match=1877 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.370 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.364 n_q1=432 n_q2=499 n_q3=447 n_q4=499 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits'
Saving the final (post-refit) wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits sigma_overall=0.367 worst_q_ratio=1.104
new2=fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits sigma_overall=0.375 worst_q_ratio=1.144
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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414_astrometric_residuals.png (1893 matched stars from wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415_astrometric_residuals.png (1877 matched stars from wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits'
Saving fully-calibrated image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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 00:26:52.99 -05:30:59.1: 9.97 +/- 0.00 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:26:52.99 -05:30:59.1: 10.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.00 +/- 0.00
Forced photometry filter REJECTED candidate at 00:26:52.99 -05:30:59.1: ref_mag=10.00 +/- 0.00 new_mean_mag=10.1478 delta=-0.15 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20269_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 20269_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20274_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 20274_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03946_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 03946_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 23:44:04.82 +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: 2s
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 ####
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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits exists and is non-empty
wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Image size: 941.4'x626.8' 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: 23:59:57.600 -02:00:49.56 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 23:59:57.600 -02:00:49.56
Angular distance between the image centers 0.0147 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
Image size: 941.4'x626.8' 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: 23:59:54.990 -02:00:49.45 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 23:59:54.990 -02:00:49.45
Angular distance between the image centers 0.0243 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 23:59:57.600 -02:00:49.56
Second-epoch second image center 23:59:54.990 -02:00:49.45
Angular distance between the image centers 0.01087 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.IdnlVM6ZEv
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.QAB62Bbyvg
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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits &> /tmp/tmp.AZmq7Htqa7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits &> /tmp/tmp.tnDKX5eWaN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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 25 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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
2.0 pix fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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
14.1 mag. fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
14.1 mag. fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.5 (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.IdnlVM6ZEv (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/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.QAB62Bbyvg (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/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.AZmq7Htqa7 (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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=4, blended=515, bad_region=0, passed=15793
Got 15793 stars (including 15246 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat
util/solve_plate_with_UCAC5 got 15793 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8565 through 0 to 8.1421, gap 8.1421 to 351.8565
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 -7.7 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
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 15793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 351.8562 through 0 to 8.1428, gap 8.1428 to 351.8562
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 -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 15793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 15793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4880 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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=4880 robust_rms=10.110 arcsec worst_quadrant_rms=10.641 arcsec
SIP_REFIT: SIP order 3 trial: matched=4880 robust_rms=0.556 arcsec worst_quadrant_rms=0.594 arcsec
SIP_REFIT: SIP order 5 trial: matched=4880 robust_rms=0.412 arcsec worst_quadrant_rms=0.433 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4880 robust_rms_before=1.043 arcsec robust_rms_before_corrected=0.400 arcsec robust_rms_after=0.412 arcsec worst_quadrant_rms_before=0.432 worst_quadrant_rms_after=0.433
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.432 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits N_match=4880 sigma_overall_arcsec=0.408 sigma_q1_arcsec=0.424 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.398 sigma_q4_arcsec=0.374 n_q1=1242 n_q2=1267 n_q3=1154 n_q4=1217 worst_quadrant_to_overall_ratio=1.050
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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.tnDKX5eWaN (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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
Checking if the catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits
WCS catalog name: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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=6, blended=513, bad_region=0, passed=15812
Got 15812 stars (including 15267 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat
util/solve_plate_with_UCAC5 got 15812 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8052 through 0 to 8.1421, gap 8.1421 to 351.8052
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 -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 4880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 15812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 351.8049 through 0 to 8.1427, gap 8.1427 to 351.8049
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 -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 15812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 15812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4881 stars left (next iteration limit 5368)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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=4881 robust_rms=9.887 arcsec worst_quadrant_rms=10.405 arcsec
SIP_REFIT: SIP order 3 trial: matched=4881 robust_rms=0.568 arcsec worst_quadrant_rms=0.590 arcsec
SIP_REFIT: SIP order 5 trial: matched=4881 robust_rms=0.415 arcsec worst_quadrant_rms=0.436 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4881 robust_rms_before=1.056 arcsec robust_rms_before_corrected=0.412 arcsec robust_rms_after=0.415 arcsec worst_quadrant_rms_before=0.445 worst_quadrant_rms_after=0.436
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.445 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits N_match=4881 sigma_overall_arcsec=0.410 sigma_q1_arcsec=0.430 sigma_q2_arcsec=0.438 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.387 n_q1=1239 n_q2=1267 n_q3=1160 n_q4=1215 worst_quadrant_to_overall_ratio=1.069
The image catalog is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits -region wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-20-12_20.00sec_-0.00C_LIGHTs_0414.fits
Saving fully-calibrated image wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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_2026-09-01_CI_Psc-08-Q1b1x1_042335_TTUQ1b1x1_2282068_41zaaBSU/wcs_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415.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 00:08:22.35 -06:16:58.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:49:56.11 +01:54:08.3: 12.67 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:17:39.30 -01:01:19.7: 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 00:14:06.98 -06:55:56.6: 12.51 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:40:03.09 +02:51:52.1: 12.05 +/- 0.01 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:59:45.73 -05:52:34.2: 12.36 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:17:21.00 -01:30:27.1: 15.79 +/- 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 -05:30:59.2: 10.20 +/- 0.00 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:54:09.52 +02:19:04.4: 12.22 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:40:03.09 +02:51:52.1: 12.03 +/- 0.01 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:49:56.11 +01:54:08.3: 12.70 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:59:45.73 -05:52:34.2: 12.39 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:17:21.00 -01:30:27.1: 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 00:08:22.35 -06:16:58.6: 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 23:54:09.52 +02:19:04.4: 12.23 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:17:39.30 -01:01:19.7: 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 00:14:06.98 -06:55:56.6: 12.48 +/- 0.02 detection
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 -05:30:59.2: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry filter REJECTED candidate at 23:59:45.73 -05:52:34.2: ref_mag=12.37 +/- 0.01 new_mean_mag=12.4196 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:49:56.11 +01:54:08.3: ref_mag=12.68 +/- 0.02 new_mean_mag=12.9508 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:40:03.09 +02:51:52.1: ref_mag=12.04 +/- 0.01 new_mean_mag=12.2149 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:14:06.98 -06:55:56.6: ref_mag=12.50 +/- 0.01 new_mean_mag=12.9434 delta=-0.45 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:17:39.30 -01:01:19.7: ref_mag=12.65 +/- 0.02 new_mean_mag=13.0921 delta=-0.44 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:54:09.52 +02:19:04.4: ref_mag=12.22 +/- 0.01 new_mean_mag=12.4969 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:26:53.02 -05:30:59.2: ref_mag=10.23 +/- 0.00 new_mean_mag=10.2006 delta=0.03 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:38:24.46 +01:55:17.5: 12.43 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:28:28.16 -03:35:37.2: 13.19 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:45:11.96 +02:18:06.8: 12.40 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:00:37.84 -01:04:07.7: 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 00:10:44.18 +02:02:36.5: 13.17 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:35:56.29 +02:25:58.9: 12.86 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:43:10.53 +00:29:00.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:28:28.16 -03:35:37.2: 13.12 +/- 0.04 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 +02:18:06.8: 12.49 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:00:37.84 -01:04:07.7: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:38:24.46 +01:55:17.5: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 00:28:28.16 -03:35:37.2: ref_mag=13.15 +/- 0.03 new_mean_mag=12.8347 delta=0.32 (need > 0.90)
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter REJECTED candidate at 23:45:11.96 +02:18:06.8: ref_mag=12.44 +/- 0.01 new_mean_mag=12.6375 delta=-0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:38:24.46 +01:55:17.5: ref_mag=12.43 +/- 0.01 new_mean_mag=12.5759 delta=-0.14 (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 +02:02:26.3: 13.21 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:10:44.18 +02:02:36.5: 13.08 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:35:56.29 +02:25:58.9: 12.89 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:43:10.53 +00:29:00.8: 15.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter REJECTED candidate at 23:35:56.29 +02:25:58.9: ref_mag=12.88 +/- 0.02 new_mean_mag=13.0461 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:10:44.18 +02:02:36.5: ref_mag=13.12 +/- 0.03 new_mean_mag=13.1228 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:47:44.00 +02:02:26.3: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry filter REJECTED candidate at 23:47:44.00 +02:02:26.3: ref_mag=13.22 +/- 0.03 new_mean_mag=13.2274 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:38:22.52 +00:34:20.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:48:23.45 -02:01:04.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:49:39.37 -01:22:05.8: 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 23:38:22.52 +00:34:20.5: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q1b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:48:23.45 -02:01:04.7: 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 23:49:39.37 -01:22:05.8: 15.77 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out32904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33421.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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 32779_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 32779_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 32780_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 32780_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 32781_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 32781_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 32782_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 32782_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 32784_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 32784_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 32789_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 32789_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 32904_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 32904_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 32980_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 32980_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33036_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33036_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33044_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 33044_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 33046_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33046_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:26:59.30 -06:35:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33054_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33054_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33066_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33066_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33069_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33069_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 23:29:32.39 -01:46:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33091_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 33091_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 33104_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33104_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33147_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33147_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 23:54:52.14 +00:04:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33148_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33148_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33211_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33211_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33274_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 33274_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 33291_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 33291_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 33297_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 33297_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 33338_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 33338_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 33421_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
Preparing report for the candidate 33421_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
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Considering the candidate 26990_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415
The candidate 26990_fd_Psc-08-Q1b1x1_2026-09-01_04-21-19_20.00sec_0.00C_LIGHTs_0415 did not pass the final checks
