This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 17.3697 2461269.8698 11.56 23:34:48.48 +02:57:46.8
88.39342 -54.68700 galactic Psc Second-epoch detections are separated by 0.5" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.236 Honoria 0 -0 0 11.4 -0 -0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:34:48.48 +02:57:46.8: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:34:48.48 +02:57:46.8: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.8698,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3697 11.56CV 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 08 17.3697 2461269.8698 12.72 23:37:49.39 +05:47:30.9
91.81152 -52.57440 galactic Psc Second-epoch detections are separated by 0.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.338 Budrosa -0 0 0 13.1 0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:37:49.39 +05:47:30.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:37:49.39 +05:47:30.9: 15.74 +/- 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,2461269.8698,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3697 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3697 2461269.8698 12.62 00:19:48.36 +00:55:47.6
106.48624 -60.92783 galactic Psc Second-epoch detections are separated by 0.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.217 Eudora -0 1 1 12.7 0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:19:48.36 +00:55:47.6: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:19:48.36 +00:55:47.6: 15.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.8698,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3697 12.62CV 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 08 17.3697 2461269.8698 13.61 23:50:41.84 +01:17:03.5
93.27416 -58.04648 galactic Psc Second-epoch detections are separated by 2.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.570 Kythera -1 -0 1 13.7 0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:50:41.84 +01:17:03.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:50:41.84 +01:17:03.5: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.8698,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3697 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3697 2461269.8698 13.66 23:46:23.15 +02:11:55.4
92.24551 -56.74656 galactic Psc Second-epoch detections are separated by 3.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.788 Hohensteina 0 2 2 13.9 -0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:46:23.15 +02:11:55.4: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:46:23.15 +02:11:55.4: 15.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.8698,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3697 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3697 2461269.8698 13.91 23:35:18.69 +08:51:03.7
93.14336 -49.56666 galactic Peg Second-epoch detections are separated by 1.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.552 Sigelinde -2 -1 2 14.6 0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:35:18.69 +08:51:03.7: 15.32 +/- 0.26 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:35:18.69 +08:51:03.7: 15.69 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.32 +/- 0.26
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,2461269.8698,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3697 13.91CV 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 08 17.3697 2461269.8698 14.34 23:49:30.26 +08:55:02.1
98.18188 -50.95403 galactic Peg Second-epoch detections are separated by 1.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1353 Maartje -1 0 1 14.4 -0 -0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:49:30.26 +08:55:02.1: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:49:30.26 +08:55:02.1: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.8698,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3697 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
First image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Last image: 2461269.87004330 17.08.2026 08:52:41.741 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 6704
Objects passed selection criteria: 6701
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6469
Average stars matched: 6166 (95.3161 %)
Memory usage VmPeak: 232876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 03:56:54 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
First image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Last image: 2461269.87004330 17.08.2026 08:52:41.741 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 36
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 31877
Objects passed selection criteria: 31811
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 30480.2
Average stars matched: 29250.2 (95.9646 %)
Memory usage VmPeak: 255820 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 03:57:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.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: 2461269.86945675
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits exists and is non-empty
wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.228 +05:59:38.82 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.149 +05:58:49.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:01.149 +05:58:49.27
Angular distance between the image centers 0.0183 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Image size: 940.8'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 00:00:02.658 +05:58:09.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:02.658 +05:58:09.64
Angular distance between the image centers 0.0308 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 00:00:01.149 +05:58:49.27
Second-epoch second image center 00:00:02.658 +05:58:09.64
Angular distance between the image centers 0.01266 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits &> /tmp/tmp.RaVxbWQFgH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits &> /tmp/tmp.hzjCzM2qoj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits &> /tmp/tmp.RS94hADatx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits &> /tmp/tmp.U99GA2Yf5d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 6233 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.0271 to 7.9045 deg, Dec +0.6902 to +11.2647 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.0271 to 7.9045 deg, Dec 0.6902 to 11.2647 deg
Loaded 4566 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): 3722 out of 3826 total matches.
Matched with Tycho-2 3826 out of 6233 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.662650
a=0.000000 b=1.000000 c=22.662650
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 6233 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.0271 to 7.9045 deg, Dec +0.6902 to +11.2647 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.0271 to 7.9045 deg, Dec 0.6902 to 11.2647 deg
Loaded 4566 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): 3722 out of 3826 total matches.
Matched with Tycho-2 3826 out of 6233 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (aperture=6.4)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 6318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.8996 to 8.2591 deg, Dec +0.3478 to +11.6137 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 351.8996 to 8.2591 deg, Dec 0.3478 to 11.6137 deg
Loaded 4984 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): 3763 out of 3845 total matches.
Matched with Tycho-2 3845 out of 6318 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
2.4 pix Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
3.8 pix fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
3.8 pix fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Limiting magnitude estimates:
15.1 mag. Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
15.1 mag. Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
14.9 mag. fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
14.9 mag. fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.RaVxbWQFgH (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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=357, bad_region=0, passed=6233
Got 6233 stars (including 5867 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
util/solve_plate_with_UCAC5 got 6233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0271 through 0 to 7.9045, gap 7.9045 to 352.0271
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0274 through 0 to 7.9045, gap 7.9045 to 352.0274
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4897 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits N_match=4897 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.420 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.391 n_q1=1279 n_q2=1239 n_q3=1222 n_q4=1157 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -region wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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.hzjCzM2qoj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=328, bad_region=0, passed=6318
Got 6318 stars (including 5982 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
util/solve_plate_with_UCAC5 got 6318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8996 through 0 to 8.2591, gap 8.2591 to 351.8996
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8998 through 0 to 8.2592, gap 8.2592 to 351.8998
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4892 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits N_match=4892 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.300 sigma_q4_arcsec=0.304 n_q1=1292 n_q2=1193 n_q3=1278 n_q4=1129 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -region wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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.RS94hADatx (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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=248, bad_region=0, passed=6740
Got 6740 stars (including 6488 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat
util/solve_plate_with_UCAC5 got 6740 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8763 through 0 to 8.2373, gap 8.2373 to 351.8763
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 6740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8757 through 0 to 8.2376, gap 8.2376 to 351.8757
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4894 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4894 robust_rms=10.853 arcsec worst_quadrant_rms=12.277 arcsec
SIP_REFIT: SIP order 3 trial: matched=4894 robust_rms=0.376 arcsec worst_quadrant_rms=0.396 arcsec
SIP_REFIT: SIP order 5 trial: matched=4894 robust_rms=0.314 arcsec worst_quadrant_rms=0.349 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4894 robust_rms_before=0.841 arcsec robust_rms_before_corrected=0.296 arcsec robust_rms_after=0.314 arcsec worst_quadrant_rms_before=0.342 worst_quadrant_rms_after=0.349
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.342 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits N_match=4894 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.331 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.245 n_q1=1252 n_q2=1182 n_q3=1292 n_q4=1168 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits -region wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.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.U99GA2Yf5d (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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=256, bad_region=0, passed=6733
Got 6733 stars (including 6475 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat
util/solve_plate_with_UCAC5 got 6733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9007 through 0 to 8.2372, gap 8.2372 to 351.9007
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 6733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9000 through 0 to 8.2375, gap 8.2375 to 351.9000
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4892 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4892 robust_rms=10.828 arcsec worst_quadrant_rms=12.611 arcsec
SIP_REFIT: SIP order 3 trial: matched=4892 robust_rms=0.375 arcsec worst_quadrant_rms=0.381 arcsec
SIP_REFIT: SIP order 5 trial: matched=4892 robust_rms=0.311 arcsec worst_quadrant_rms=0.347 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4892 robust_rms_before=0.816 arcsec robust_rms_before_corrected=0.300 arcsec robust_rms_after=0.311 arcsec worst_quadrant_rms_before=0.349 worst_quadrant_rms_after=0.347
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.349 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits N_match=4892 sigma_overall_arcsec=0.298 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.349 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.259 n_q1=1252 n_q2=1183 n_q3=1302 n_q4=1155 worst_quadrant_to_overall_ratio=1.170
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits -region wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits'
Saving the final (post-refit) wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits'
Saving the final (post-refit) wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits'
Saving the final (post-refit) wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits sigma_overall=0.375 worst_q_ratio=1.120
ref2=Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits sigma_overall=0.303 worst_q_ratio=1.077
new1=fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits sigma_overall=0.294 worst_q_ratio=1.156
new2=fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits sigma_overall=0.298 worst_q_ratio=1.170
reference average sigma_overall=0.339 worst_q_ratio=1.0985
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966_astrometric_residuals.png (4897 matched stars from wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382_astrometric_residuals.png (4892 matched stars from wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388_astrometric_residuals.png (4894 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389_astrometric_residuals.png (4892 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits'
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits'
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:03:30.74 +04:49:48.0: 12.16 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:34:48.48 +02:57:46.8: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:56:45.71 +05:39:18.8: 12.24 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:03:30.74 +04:49:48.0: 12.22 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:56:45.71 +05:39:18.8: 12.28 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:34:48.48 +02:57:46.8: 15.54 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter REJECTED candidate at 00:03:30.74 +04:49:48.0: ref_mag=12.19 +/- 0.01 new_mean_mag=12.1611 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:56:45.71 +05:39:18.8: ref_mag=12.26 +/- 0.01 new_mean_mag=12.2146 delta=0.05 (need > 0.90)
Adding exclusion_list_local.txt__out20600.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 20600_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
Preparing report for the candidate 20600_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
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Considering the candidate 20602_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 20602_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
**** FOUND 23:36:10.46 +09:48:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20607_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 20607_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
**** FOUND 23:51:22.71 +09:20:48.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20609_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 20609_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 20610_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 20610_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 20611_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 20611_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:34:48.48 +02:57:46.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits exists and is non-empty
wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.228 +05:59:38.82 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.149 +05:58:49.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:01.149 +05:58:49.27
Angular distance between the image centers 0.0183 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Image size: 940.8'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 00:00:02.658 +05:58:09.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:02.658 +05:58:09.64
Angular distance between the image centers 0.0308 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 00:00:01.149 +05:58:49.27
Second-epoch second image center 00:00:02.658 +05:58:09.64
Angular distance between the image centers 0.01266 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits &> /tmp/tmp.7LWCFXNVb7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits &> /tmp/tmp.pnlWq3yCIL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits &> /tmp/tmp.XlwyTXgbx5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits &> /tmp/tmp.FACtq0esZK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33634 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9992 to 7.9160 deg, Dec +0.6902 to +11.2656 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 351.9992 to 7.9160 deg, Dec 0.6902 to 11.2656 deg
Loaded 4573 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): 3677 out of 3960 total matches.
Matched with Tycho-2 3960 out of 33634 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.546200
a=0.000000 b=1.000000 c=22.546200
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33634 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9992 to 7.9160 deg, Dec +0.6902 to +11.2656 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 351.9992 to 7.9160 deg, Dec 0.6902 to 11.2656 deg
Loaded 4573 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): 3677 out of 3960 total matches.
Matched with Tycho-2 3960 out of 33634 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (aperture=5.0)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33762 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.8996 to 8.2739 deg, Dec +0.3067 to +11.6461 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 351.8996 to 8.2739 deg, Dec 0.3067 to 11.6461 deg
Loaded 5018 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): 3715 out of 3975 total matches.
Matched with Tycho-2 3975 out of 33762 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
2.4 pix Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
3.4 pix fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
3.4 pix fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Limiting magnitude estimates:
15.2 mag. Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
15.2 mag. Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
14.9 mag. fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
14.9 mag. fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.7LWCFXNVb7 (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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1340, bad_region=0, passed=33612
Got 33612 stars (including 32227 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
util/solve_plate_with_UCAC5 got 33612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9992 through 0 to 7.9160, gap 7.9160 to 351.9992
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 33612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9998 through 0 to 7.9160, gap 7.9160 to 351.9998
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 33612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 33612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4893 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits N_match=4893 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.369 n_q1=1276 n_q2=1249 n_q3=1197 n_q4=1171 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -region wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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.pnlWq3yCIL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1193, bad_region=21, passed=33746
Got 33746 stars (including 32487 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
util/solve_plate_with_UCAC5 got 33746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8996 through 0 to 8.2739, gap 8.2739 to 351.8996
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 33746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8999 through 0 to 8.2739, gap 8.2739 to 351.8999
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 33746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 33746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits N_match=4885 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.267 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.298 n_q1=1273 n_q2=1211 n_q3=1272 n_q4=1129 worst_quadrant_to_overall_ratio=1.059
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -region wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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.XlwyTXgbx5 (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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1077, bad_region=45, passed=27759
Got 27759 stars (including 26609 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat
util/solve_plate_with_UCAC5 got 27759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8715 through 0 to 8.2731, gap 8.2731 to 351.8715
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 4891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 27759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8709 through 0 to 8.2734, gap 8.2734 to 351.8709
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 27759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 27759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4891 stars left (next iteration limit 5380)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4891 robust_rms=11.158 arcsec worst_quadrant_rms=12.342 arcsec
SIP_REFIT: SIP order 3 trial: matched=4891 robust_rms=0.379 arcsec worst_quadrant_rms=0.408 arcsec
SIP_REFIT: SIP order 5 trial: matched=4891 robust_rms=0.312 arcsec worst_quadrant_rms=0.344 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4891 robust_rms_before=0.837 arcsec robust_rms_before_corrected=0.294 arcsec robust_rms_after=0.312 arcsec worst_quadrant_rms_before=0.340 worst_quadrant_rms_after=0.344
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.340 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits N_match=4891 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.255 sigma_q4_arcsec=0.247 n_q1=1232 n_q2=1172 n_q3=1305 n_q4=1182 worst_quadrant_to_overall_ratio=1.172
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits -region wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.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.FACtq0esZK (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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1107, bad_region=45, passed=27777
Got 27777 stars (including 26596 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat
util/solve_plate_with_UCAC5 got 27777 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8915 through 0 to 8.2731, gap 8.2731 to 351.8915
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 27777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8908 through 0 to 8.2733, gap 8.2733 to 351.8908
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 27777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 27777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4893 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4893 robust_rms=11.253 arcsec worst_quadrant_rms=12.424 arcsec
SIP_REFIT: SIP order 3 trial: matched=4893 robust_rms=0.380 arcsec worst_quadrant_rms=0.384 arcsec
SIP_REFIT: SIP order 5 trial: matched=4893 robust_rms=0.310 arcsec worst_quadrant_rms=0.346 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4893 robust_rms_before=0.812 arcsec robust_rms_before_corrected=0.302 arcsec robust_rms_after=0.310 arcsec worst_quadrant_rms_before=0.352 worst_quadrant_rms_after=0.346
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.352 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits N_match=4893 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.265 n_q1=1226 n_q2=1175 n_q3=1298 n_q4=1194 worst_quadrant_to_overall_ratio=1.163
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits -region wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.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-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-51-51_20.00sec_-0.00C_LIGHTs_0388.fits
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.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_2026-08-17_CI_Psc-04-Q1b1x1_035319_TTUQ1b1x1_3035790_XVun1NLv/wcs_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389.fits
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:55:07.58 +11:09:36.7: 13.83 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:01:42.21 +09:27:41.6: 14.51 +/- 0.10 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:37:49.39 +05:47:30.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:35:18.69 +08:51:03.7: 15.32 +/- 0.26 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:50:41.84 +01:17:03.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:30:12.34 +04:01:54.1: 13.74 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:46:23.15 +02:11:55.4: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:19:48.36 +00:55:47.6: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:55:17.56 +05:05:31.0: 14.07 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:26:12.42 +07:38:14.3: 14.20 +/- 0.08 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:55:07.58 +11:09:36.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:35:18.69 +08:51:03.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:01:42.21 +09:27:41.6: 14.58 +/- 0.11 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:55:17.56 +05:05:31.0: 14.14 +/- 0.07 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:50:41.84 +01:17:03.5: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:37:49.39 +05:47:30.9: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:46:23.15 +02:11:55.4: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:19:48.36 +00:55:47.6: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:30:12.34 +04:01:54.1: 13.81 +/- 0.07 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.26
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry reference-image weighted average: 14.54 +/- 0.08
Forced photometry filter KEPT candidate at 23:35:18.69 +08:51:03.7: ref_mag=15.32 +/- 0.26 new_mean_mag=13.8808 delta=1.44 (need > 0.90)
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Forced photometry filter REJECTED candidate at 23:55:07.58 +11:09:36.7: ref_mag=13.79 +/- 0.04 new_mean_mag=14.1808 delta=-0.39 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:01:42.21 +09:27:41.6: ref_mag=14.54 +/- 0.08 new_mean_mag=14.5817 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:55:17.56 +05:05:31.0: ref_mag=14.10 +/- 0.05 new_mean_mag=14.1899 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Forced photometry filter REJECTED candidate at 23:30:12.34 +04:01:54.1: ref_mag=13.78 +/- 0.05 new_mean_mag=14.0809 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:26:12.42 +07:38:14.3: 14.32 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Forced photometry filter REJECTED candidate at 00:26:12.42 +07:38:14.3: ref_mag=14.25 +/- 0.06 new_mean_mag=14.0863 delta=0.16 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:28:16.76 +07:42:20.3: 14.67 +/- 0.14 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:49:30.26 +08:55:02.1: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:51:45.68 +11:12:17.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:30:36.41 +10:13:36.8: 14.73 +/- 0.17 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:30:14.84 +08:53:22.7: 14.79 +/- 0.17 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:28:16.76 +07:42:20.3: 15.08 +/- 0.21 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:30:36.41 +10:13:36.8: 14.95 +/- 0.21 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:49:30.26 +08:55:02.1: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:51:45.68 +11:12:17.7: 14.86 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 23:51:45.68 +11:12:17.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 14.79 +/- 0.12
Forced photometry reference-image weighted average: 14.81 +/- 0.13
Forced photometry filter REJECTED candidate at 00:28:16.76 +07:42:20.3: ref_mag=14.79 +/- 0.12 new_mean_mag=14.4165 delta=0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:30:36.41 +10:13:36.8: ref_mag=14.81 +/- 0.13 new_mean_mag=14.5015 delta=0.31 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:30:14.84 +08:53:22.7: 15.05 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.14
Forced photometry filter REJECTED candidate at 23:30:14.84 +08:53:22.7: ref_mag=14.89 +/- 0.14 new_mean_mag=14.5748 delta=0.31 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:30:38.14 +09:10:15.8: 14.90 +/- 0.19 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:03:05.28 +10:23:11.5: 14.62 +/- 0.12 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:29:31.40 +10:14:33.1: 14.85 +/- 0.18 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:52:52.45 +10:04:13.5: 14.66 +/- 0.12 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:30:38.14 +09:10:15.8: 14.89 +/- 0.19 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:29:31.40 +10:14:33.1: 14.97 +/- 0.21 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:03:05.28 +10:23:11.5: 14.63 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.13
Forced photometry filter REJECTED candidate at 00:30:38.14 +09:10:15.8: ref_mag=14.90 +/- 0.13 new_mean_mag=14.5087 delta=0.39 (need > 0.90)
Forced photometry reference-image weighted average: 14.62 +/- 0.08
Forced photometry reference-image weighted average: 14.90 +/- 0.13
Forced photometry filter REJECTED candidate at 00:03:05.28 +10:23:11.5: ref_mag=14.62 +/- 0.08 new_mean_mag=14.5485 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:29:31.40 +10:14:33.1: ref_mag=14.90 +/- 0.13 new_mean_mag=14.6975 delta=0.20 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:52:52.45 +10:04:13.5: 14.73 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.09
Forced photometry filter REJECTED candidate at 23:52:52.45 +10:04:13.5: ref_mag=14.69 +/- 0.09 new_mean_mag=14.6403 delta=0.05 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:28:48.30 +08:53:58.6: 14.90 +/- 0.17 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:30:19.85 +08:34:03.7: 14.95 +/- 0.18 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:17:24.49 +10:46:42.9: 15.48 +/- 0.27 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:51:47.09 +10:14:30.1: 14.97 +/- 0.16 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:17:24.49 +10:46:42.9: 15.07 +/- 0.19 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:28:48.30 +08:53:58.6: 15.01 +/- 0.19 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:30:19.85 +08:34:03.7: 14.95 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.15
Forced photometry reference-image weighted average: 14.94 +/- 0.13
Forced photometry reference-image weighted average: 14.95 +/- 0.13
Forced photometry filter REJECTED candidate at 00:28:48.30 +08:53:58.6: ref_mag=14.94 +/- 0.13 new_mean_mag=14.7227 delta=0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:17:24.49 +10:46:42.9: ref_mag=15.20 +/- 0.15 new_mean_mag=14.8126 delta=0.39 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:30:19.85 +08:34:03.7: ref_mag=14.95 +/- 0.13 new_mean_mag=14.7629 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:51:47.09 +10:14:30.1: 14.94 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.11
Forced photometry filter REJECTED candidate at 23:51:47.09 +10:14:30.1: ref_mag=14.95 +/- 0.11 new_mean_mag=14.7758 delta=0.18 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:26:42.79 +07:53:20.6: 15.11 +/- 0.19 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:28:23.74 +05:10:45.5: 14.74 +/- 0.14 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:14:34.98 +08:10:52.5: 15.43 +/- 0.24 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:18:27.31 +03:50:19.2: 15.06 +/- 0.19 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:26:42.79 +07:53:20.6: 15.06 +/- 0.19 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:28:23.74 +05:10:45.5: 15.07 +/- 0.21 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:14:34.98 +08:10:52.5: 15.22 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.14
Forced photometry reference-image weighted average: 14.84 +/- 0.12
Forced photometry filter REJECTED candidate at 00:26:42.79 +07:53:20.6: ref_mag=15.09 +/- 0.14 new_mean_mag=14.6341 delta=0.45 (need > 0.90)
Forced photometry reference-image weighted average: 15.31 +/- 0.16
Forced photometry filter REJECTED candidate at 00:28:23.74 +05:10:45.5: ref_mag=14.84 +/- 0.12 new_mean_mag=14.6880 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:14:34.98 +08:10:52.5: ref_mag=15.31 +/- 0.16 new_mean_mag=14.6906 delta=0.62 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:18:27.31 +03:50:19.2: 15.17 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.14
Forced photometry filter REJECTED candidate at 00:18:27.31 +03:50:19.2: ref_mag=15.11 +/- 0.14 new_mean_mag=14.6588 delta=0.45 (need > 0.90)
Adding exclusion_list_local.txt__out53745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53944.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 45s
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 53692_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53692_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 53693_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53693_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 53696_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53696_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 53702_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53702_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 53717_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53717_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
**** FOUND 23:34:48.48 +02:57:46.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53745_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
Preparing report for the candidate 53745_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
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Considering the candidate 53746_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
Preparing report for the candidate 53746_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
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Considering the candidate 53814_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
Preparing report for the candidate 53814_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
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Considering the candidate 53848_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
Preparing report for the candidate 53848_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
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Considering the candidate 53874_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
Preparing report for the candidate 53874_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
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Considering the candidate 53903_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53903_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 53944_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
Preparing report for the candidate 53944_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
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Considering the candidate 53955_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53955_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 53966_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53966_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 53969_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 53969_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54012_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54012_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54018_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54018_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54025_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54025_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54033_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54033_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54046_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54046_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54056_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54056_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54060_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54060_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54065_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54065_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54068_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54068_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54080_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54080_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54094_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54094_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54095_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54095_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 54137_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 54137_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
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Considering the candidate 23891_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 23891_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
**** FOUND 23:54:22.29 +07:22:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26495_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389
The candidate 26495_fd_Psc-04-Q1b1x1_2026-08-17_03-52-41_20.00sec_-0.00C_LIGHTs_0389 did not pass the final checks
