This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1
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,2461214.8735,7.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 7.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461214.8735,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 8.79CV 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 06 23.3735 2461214.8735 10.13 01:01:56.71 +03:45:37.5
128.02718 -59.00734 galactic Psc Second-epoch detections are separated by 1.0" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2 Pallas -0 -0 0 10.0 0 0
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:01:56.71 +03:45:37.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:01:56.71 +03:45:37.5: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461214.8735,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 10.13CV 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,2461214.8735,6.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 6.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461214.8735,8.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 8.57CV 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 06 23.3735 2461214.8735 12.56 00:58:40.80 +07:36:27.2
126.07901 -55.21993 galactic Psc Second-epoch detections are separated by 0.7" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.101 Helena -1 -1 1 13.1 -0 -0
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:58:40.80 +07:36:27.2: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:58:40.80 +07:36:27.2: 16.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461214.8735,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 12.56CV 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 06 23.3735 2461214.8735 12.76 00:55:24.49 +06:32:09.7
124.71041 -56.32201 galactic Psc Second-epoch detections are separated by 0.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -0 -0 0 13.0 -0 -0
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:24.49 +06:32:09.7: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:24.49 +06:32:09.7: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461214.8735,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 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 06 23.3735 2461214.8735 13.35 00:54:52.13 +09:15:31.0
124.35870 -53.60363 galactic Psc Second-epoch detections are separated by 0.7" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.385 Ilmatar -0 -1 1 13.9 -0 -0
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:54:52.13 +09:15:31.0: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:54:52.13 +09:15:31.0: 16.06 +/- 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,2461214.8735,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 23.3735 2461214.8735 13.31 01:06:34.54 +07:39:44.7
129.48319 -55.01666 galactic Psc Second-epoch detections are separated by 1.5" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.124 Alkeste 0 -0 0 13.5 0 0
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:06:34.54 +07:39:44.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:06:34.54 +07:39:44.7: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461214.8735,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 13.31CV 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 06 23.3735 2461214.8735 13.74 01:04:43.79 +10:06:05.8
128.32689 -52.63085 galactic Psc Second-epoch detections are separated by 1.2" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.212 Medea -0 -1 1 14.2 -0 -0
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:04:43.79 +10:06:05.8: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:04:43.79 +10:06:05.8: 16.00 +/- 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,2461214.8735,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260623.3735 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
First image: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Last image: 2461214.87377213 23.06.2026 08:58:03.912 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5028
Objects passed selection criteria: 5000
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 3351
Average stars matched: 3137.75 (93.6362 %)
Memory usage VmPeak: 111296 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 21 14:44:16 CDT 2026
VaST build number 1.0rc89-107-g3b0f95a5
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 23 04:59:02 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
First image: 2461049.62262976 09.01.2026 02:56:25.211 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Last image: 2461214.87377213 23.06.2026 08:58:03.912 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 28974
Objects passed selection criteria: 28907
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 20312.5
Average stars matched: 18837 (92.736 %)
Memory usage VmPeak: 131460 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 21 14:44:16 CDT 2026
VaST build number 1.0rc89-107-g3b0f95a5
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 23 05:01:03 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/TTUQ2b1x1/TTUQ2_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 --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
SExtractor catalog cache: saved Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.cat to cache
SExtractor catalog cache: saved Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.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: 2461214.87322313
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits exists and is non-empty
Saving wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits to local_wcs_cache/
'wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits' -> 'local_wcs_cache/wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits'
wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits exists and is non-empty
Saving wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits to local_wcs_cache/
'wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits'
wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits exists and is non-empty
Saving wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits to local_wcs_cache/
'wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits' -> 'local_wcs_cache/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits'
wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits exists and is non-empty
Saving wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits to local_wcs_cache/
'wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits' -> 'local_wcs_cache/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (1st reference image)
verification OK: wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:32.310 +05:59:46.72 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits (1st new image)
verification OK: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Image size: 938.7'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:51:20.619 +06:04:05.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:20.619 +06:04:05.76
Angular distance between the image centers 0.0867 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits (2nd new image)
verification OK: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Image size: 938.7'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:51:23.848 +06:04:40.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:23.848 +06:04:40.21
Angular distance between the image centers 0.0887 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 00:51:20.619 +06:04:05.76
Second-epoch second image center 00:51:23.848 +06:04:40.21
Angular distance between the image centers 0.01645 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits &> /tmp/tmp.fK4CiWmvn1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.MxV6GbE2VX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits &> /tmp/tmp.Ij5MjXgd7G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits &> /tmp/tmp.51QO1WvuQ1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Found non-empty wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
The reference image (wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits) and catalog (wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat) found
'wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat' -> 'wcsmag.cat'
Read 6274 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.9081 to 20.8681 deg, Dec +0.7095 to +11.2754 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 4.9081 to 20.8681 deg, Dec 0.7095 to 11.2754 deg
Loaded 4466 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): 3642 out of 3799 total matches.
Matched with Tycho-2 3799 out of 6274 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.870250
a=0.000000 b=1.000000 c=22.870250
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6274 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.9081 to 20.8681 deg, Dec +0.7095 to +11.2754 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 4.9081 to 20.8681 deg, Dec 0.7095 to 11.2754 deg
Loaded 4466 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): 3642 out of 3799 total matches.
Matched with Tycho-2 3799 out of 6274 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -> calib.txt_param_ref_wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (aperture=5.8)
Read 6217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8906 to 20.8646 deg, Dec +0.7094 to +11.2737 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 4.8906 to 20.8646 deg, Dec 0.7094 to 11.2737 deg
Loaded 4467 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): 3635 out of 3795 total matches.
Matched with Tycho-2 3795 out of 6217 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -> calib.txt_param_ref_wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits (aperture=5.8)
____ 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: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
2.0 pix Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
2.3 pix fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
2.3 pix fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
2.0 pix wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
2.0 pix wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Limiting magnitude estimates:
15.2 mag. Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
15.2 mag. Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
13.3 mag. fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
13.3 mag. fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
All-image limiting magnitude estimate: 13.3 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fK4CiWmvn1 (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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits' -> 'wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS-calibrated image found: wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Checking if the catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS catalog name: wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=428, bad_region=1456, passed=6274
Got 6274 stars (including 4469 good ones) from the SExtractor catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
util/solve_plate_with_UCAC5 got 6274 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 4931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 4933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 4933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits N_match=978 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.415 sigma_q2_arcsec=0.328 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.276 n_q1=271 n_q2=183 n_q3=328 n_q4=196 worst_quadrant_to_overall_ratio=1.317
The image catalog is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -region wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MxV6GbE2VX (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-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits' -> 'wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=435, bad_region=1444, passed=6217
Got 6217 stars (including 4408 good ones) from the SExtractor catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 6217 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 4914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 4913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 4913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits N_match=979 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.321 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.269 n_q1=274 n_q2=182 n_q3=328 n_q4=195 worst_quadrant_to_overall_ratio=1.358
The image catalog is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ij5MjXgd7G (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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Checking if the catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
WCS catalog name: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=151, bad_region=464, passed=2427
Got 2427 stars (including 1832 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 2427 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 980 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 2008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 2008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 2008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits N_match=981 sigma_overall_arcsec=0.398 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.405 sigma_q4_arcsec=0.421 n_q1=320 n_q2=162 n_q3=342 n_q4=157 worst_quadrant_to_overall_ratio=1.060
The image catalog is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits -region wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.51QO1WvuQ1 (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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Checking if the catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
WCS catalog name: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=137, bad_region=472, passed=2419
Got 2419 stars (including 1829 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat
util/solve_plate_with_UCAC5 got 2419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.8 to 11.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 1988 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.8 to 11.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 1987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 1987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits N_match=980 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.364 sigma_q3_arcsec=0.380 sigma_q4_arcsec=0.368 n_q1=315 n_q2=170 n_q3=344 n_q4=151 worst_quadrant_to_overall_ratio=1.025
The image catalog is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits -region wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits sigma_overall=0.315 worst_q_ratio=1.317
ref2=Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits sigma_overall=0.310 worst_q_ratio=1.358
new1=fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits sigma_overall=0.398 worst_q_ratio=1.060
new2=fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits sigma_overall=0.370 worst_q_ratio=1.025
reference average sigma_overall=0.3125 worst_q_ratio=1.3375
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069_astrometric_residuals.png (978 matched stars from wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070_astrometric_residuals.png (979 matched stars from wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366_astrometric_residuals.png (981 matched stars from wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367_astrometric_residuals.png (980 matched stars from wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits'
Saving fully-calibrated image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits'
Preparing the HTML report for the field Psc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:01:56.71 +03:45:37.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:01:56.71 +03:45:37.5: 15.87 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20440.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 20249_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 20249_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
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Considering the candidate 20288_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 20288_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
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Considering the candidate 20440_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 20440_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Psc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:01:56.71 +03:45:37.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
SExtractor catalog cache: saved Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.cat to cache
SExtractor catalog cache: saved Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Creating symlink local_wcs_cache/wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits exists and is non-empty
wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits exists and is non-empty
wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits exists and is non-empty
wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (1st reference image)
verification OK: wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:51:32.310 +05:59:46.72 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits (1st new image)
verification OK: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Image size: 938.7'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:51:20.619 +06:04:05.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:20.619 +06:04:05.76
Angular distance between the image centers 0.0867 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits (2nd new image)
verification OK: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Image size: 938.7'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:51:23.848 +06:04:40.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:51:32.310 +05:59:46.72
Second-epoch image center 00:51:23.848 +06:04:40.21
Angular distance between the image centers 0.0887 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 00:51:20.619 +06:04:05.76
Second-epoch second image center 00:51:23.848 +06:04:40.21
Angular distance between the image centers 0.01645 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits &> /tmp/tmp.OCemFjOJIQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.xhPNjt8LPL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits &> /tmp/tmp.L5zFb1tmJ1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits &> /tmp/tmp.VzNHyMehZK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Found non-empty wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits and wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
The reference image (wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits) and catalog (wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat) found
'wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat' -> 'wcsmag.cat'
Read 34129 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8906 to 20.8698 deg, Dec +0.7073 to +11.2841 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 4.8906 to 20.8698 deg, Dec 0.7073 to 11.2841 deg
Loaded 4478 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): 3588 out of 3910 total matches.
Matched with Tycho-2 3910 out of 34129 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.759600
a=0.000000 b=1.000000 c=22.759600
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34129 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8906 to 20.8698 deg, Dec +0.7073 to +11.2841 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 4.8906 to 20.8698 deg, Dec 0.7073 to 11.2841 deg
Loaded 4478 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): 3588 out of 3910 total matches.
Matched with Tycho-2 3910 out of 34129 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -> calib.txt_param_ref_wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits (aperture=4.6)
Read 34111 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 4.8822 to 20.8645 deg, Dec +0.7037 to +11.2806 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 4.8822 to 20.8645 deg, Dec 0.7037 to 11.2806 deg
Loaded 4474 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): 3580 out of 3908 total matches.
Matched with Tycho-2 3908 out of 34111 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits:
Forced-photometry filter: calibrated wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -> calib.txt_param_ref_wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
1.9 pix Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
2.1 pix fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
2.2 pix fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
1.9 pix wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
1.9 pix wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Limiting magnitude estimates:
15.4 mag. Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
15.4 mag. Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
13.9 mag. fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
13.9 mag. fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OCemFjOJIQ (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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.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-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits' -> 'wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS-calibrated image found: wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
Checking if the catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits
WCS catalog name: wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=9, blended=1306, bad_region=6510, passed=34120
Got 34120 stars (including 26507 good ones) from the SExtractor catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat
util/solve_plate_with_UCAC5 got 34120 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 28087 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 28086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 28086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits N_match=979 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.400 sigma_q2_arcsec=0.317 sigma_q3_arcsec=0.265 sigma_q4_arcsec=0.242 n_q1=274 n_q2=178 n_q3=328 n_q4=199 worst_quadrant_to_overall_ratio=1.325
The image catalog is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits -region wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xhPNjt8LPL (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-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.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-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits' -> 'wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1297, bad_region=6532, passed=34093
Got 34093 stars (including 26432 good ones) from the SExtractor catalog wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 34093 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 28151 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 28150 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 28150 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits N_match=980 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.298 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.270 n_q1=276 n_q2=175 n_q3=331 n_q4=198 worst_quadrant_to_overall_ratio=1.299
The image catalog is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.L5zFb1tmJ1 (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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Checking if the catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
WCS catalog name: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=380, bad_region=2111, passed=15390
Got 15390 stars (including 12967 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 15390 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13550 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13549 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13549 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits N_match=977 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.370 sigma_q2_arcsec=0.395 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.428 n_q1=317 n_q2=162 n_q3=335 n_q4=163 worst_quadrant_to_overall_ratio=1.093
The image catalog is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits -region wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VzNHyMehZK (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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
WCS-calibrated image found: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Checking if the catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
WCS catalog name: wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=426, bad_region=2077, passed=15398
Got 15398 stars (including 12962 good ones) from the SExtractor catalog wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat
util/solve_plate_with_UCAC5 got 15398 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13557 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits N_match=977 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.392 sigma_q4_arcsec=0.390 n_q1=318 n_q2=164 n_q3=340 n_q4=155 worst_quadrant_to_overall_ratio=1.028
The image catalog is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits -region wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-57-16_20.00sec_4.90C_LIGHT_0366.fits
Saving fully-calibrated image wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.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_2026-06-23_CI_Psc-05-Q2b1x1_041226_TTUQ2b1x1_3947846_gUrD13u1/wcs_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367.fits
Preparing the HTML report for the field Psc-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:54:52.13 +09:15:31.0: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:58:40.80 +07:36:27.2: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:57:57.59 +02:30:25.7: 12.97 +/- 0.03 detection
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:04:43.79 +10:06:05.8: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 01:06:34.54 +07:39:44.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-56-25_20.00sec_-15.00C_LIGHT_0069.fits at 00:55:24.49 +06:32:09.7: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:54:52.13 +09:15:31.0: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:58:40.80 +07:36:27.2: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:06:34.54 +07:39:44.7: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 01:04:43.79 +10:06:05.8: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:55:24.49 +06:32:09.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-05-Q2b1x1_2026-01-08_20-57-32_20.00sec_-15.00C_LIGHT_0070.fits at 00:57:57.59 +02:30:25.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter REJECTED candidate at 00:57:57.59 +02:30:25.7: ref_mag=12.99 +/- 0.02 new_mean_mag=12.8360 delta=0.15 (need > 0.90)
Adding exclusion_list_local.txt__out53542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55426.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51843_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 51843_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51882_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 51882_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52035_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
The candidate 52035_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367 did not pass the final checks
**** FOUND 01:01:56.70 +03:45:37.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53542_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 53542_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53803_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 53803_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54042_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
The candidate 54042_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54514_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 54514_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54971_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 54971_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55426_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
Preparing report for the candidate 55426_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10207_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
The candidate 10207_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367 did not pass the final checks
**** FOUND 01:02:56.22 +07:53:21.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 18371_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367
The candidate 18371_fd_Psc-05-Q2b1x1_2026-06-23_03-58-03_20.00sec_5.00C_LIGHT_0367 did not pass the final checks
